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The influence of chemical composition on models of Type Ia supernovae |
Alan C. Calder1,2( ), Brendan K. Krueger1, Aaron P. Jackson3, Dean M. Townsley4 |
| 1. Department of Physics & Astronomy, The State University of New York- Stony Brook, Stony Brook, NY 11794, USA; 2. New York Center for Computational Sciences, The State University of New York- Stony Brook, Stony Brook, NY 1794, USA; 3. National Research Council Research Associateship Program and Laboratories for Computational Physics and Fluid Dynamics, Naval Research Laboratory, Washington, DC 20375, USA; 4. Department of Physics and Astronomy, The University of Alabama, Tuscaloosa, AL 35487, USA |
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Abstract Type Ia supernovae are bright stellar explosions distinguished by standardizable light curves that allow for their use as distance indicators for cosmological studies. Despite the highly successful use of these events in this capacity, many fundamental questions remain. Contemporary research investigates how properties of the progenitor system that follow from the host galaxy such as composition and age influence the brightness of an event with the goal of better understanding and assessing the intrinsic scatter in the brightness. We provide an overview of these supernovae and proposed progenitor systems, all of which involve one or more compact stars known as white dwarfs. We describe contemporary research investigating how the composition and structure of the progenitor white dwarf systematically influences the explosion outcome assuming the progenitor is a single white dwarf that has gained mass from a companion. We present results illustrating some of these systematic effects from our research.
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| Keywords
hydrodynamics
nuclear reactions
nucleosynthesis
abundances
stars: supernovae: general
stars: white dwarfs
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Corresponding Author(s):
Calder Alan C.,Email:alan.calder@stonybrook.edu
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Issue Date: 01 April 2013
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|
| 1 |
R. Stothers, Isis. Journal of the History of Science Society , 1977, 68: 443
|
| 2 |
L. A. Marschall, The Supernova Story , New York: Plenum Press, 1988: 313
|
| 3 |
W. Baade, Astrophys. J. , 1945, 102: 309
doi: 10.1086/144761
|
| 4 |
P. Ruiz-Lapuente, Astrophys. J. , 2004, 612(1): 357
doi: 10.1086/422419
|
| 5 |
W. Baade and F. Zwicky, Phys. Rev. , 1934, 46(1): 76
doi: 10.1103/PhysRev.46.76.2
|
| 6 |
W. Hillebrandt and J. C. Niemeyer, Ann. Rev. Astron. Astrophys. , 2000, 38(1): 191
doi: 10.1146/annurev.astro.38.1.191
|
| 7 |
D. E. Osterbrock, in: American Astronomical Society Meeting Abstracts, Bull. Am. Astron. Soc. , 2001, 33: 1330
|
| 8 |
R. Minkowski, Publ. Astron. Soc. Pac. , 1941, 53: 224
doi: 10.1086/125315
|
| 9 |
F. Bertola, Annales d’Astrophysique , 1964, 27: 319
|
| 10 |
A. C. Porter and A. V. Filippenko, Astron. J. , 1987, 93: 1372
doi: 10.1086/114420
|
| 11 |
R. P. Harkness and J. C. Wheeler, in: Supernovae, edited by A. G. Petschek , 1990: 1
doi: 10.1007/978-1-4612-3286-5_1
|
| 12 |
A. V. Filippenko, Ann. Rev. Astron. Astrophys. , 1997, 35(1): 309
doi: 10.1146/annurev.astro.35.1.309
|
| 13 |
S. A. Colgate and R. H. White, Astrophys. J. , 1966, 143: 626
doi: 10.1086/148549
|
| 14 |
F. Hoyle and W. A. Fowler, Astrophys. J. , 1960, 132: 565
doi: 10.1086/146963
|
| 15 |
T. Pankey, Jr, Possible Thermonuclear Activities in Natural Terrestrial Minerals., Ph.D. thesis, Howard University , 1962
|
| 16 |
S. A. Colgate and C. McKee, Astrophys. J. , 1969, 157: 623
doi: 10.1086/150102
|
| 17 |
S. A. Colgate, A. G. Petschek, and J. T. Kriese, Astrophys. J. , 1980, 237: L81
doi: 10.1086/183239
|
| 18 |
M. J. Kuchner, R. P. Kirshner, P. A. Pinto, and B. Leibundgut, Astrophys. J. , 1994, 426: L89
doi: 10.1086/187347
|
| 19 |
I. P. Pskovskii, Sov. Astron. , 1977, 21: 675
|
| 20 |
M. M. Phillips, Astrophys. J. , 1993, 413: L105
doi: 10.1086/186970
|
| 21 |
W. D. Arnett, Astrophys. J. , 1982, 253: 785
doi: 10.1086/159681
|
| 22 |
P. A. Pinto and R. G. Eastman, Astrophys. J. , 2000, 530(2): 744
doi: 10.1086/308376
|
| 23 |
D. Kasen and S. E. Woosley, Astrophys. J. , 2007, 656(2): 661, arXiv: astro-ph/0609540
doi: 10.1086/510375
|
| 24 |
G. H. Jacoby, D. Branch, R. Ciardullo, R. L. Davies, W. E. Harris, M. J. Pierce, C. J. Pritchet, J. L. Tonry, and D. L. Welch, Publ. Astron. Soc. Pac. , 1992, 104: 599
doi: 10.1086/133035
|
| 25 |
R. P. Kirshner, arXiv: 0910.0257, 2009
|
| 26 |
F. K. R?pke, M. Gieseler, M. Reinecke, C. Travaglio, and W. Hillebrandt, Astron. Astrophys. ,2006, 453: 203, arXiv: astroph/0506107
|
| 27 |
P. H?flich, K. Krisciunas, A. M. Khokhlov, E. Baron, G. Folatelli, M. Hamuy, M. M. Phillips, N. Suntzeff, and L. Wang, Astrophys. J. , 2010, 710(1): 444, arXiv: 0912.2231
doi: 10.1088/0004-637X/710/1/444
|
| 28 |
I. R. Seitenzahl, F. Ciaraldi-Schoolmann, and F. K. R?pke, Mon. Not. R. Astron. Soc. , 2011, 414(3): 2709, arXiv: 1012.4929 [astro-ph.SR]
doi: 10.1111/j.1365-2966.2011.18588.x
|
| 29 |
I. Domíguez, P. H?flich, and O. Straniero, Astrophys. J. , 2001, 557(1): 279, arXiv: astro-ph/0104257
|
| 30 |
P. Lesaffre, Z. Han, C. A. Tout, P. Podsiadlowski, and R. G. Martin, Mon. Not. R. Astron. Soc. , 2006, 368: 187, arXiv: astroph/0601443
|
| 31 |
D. M. Townsley, A. P. Jackson, A. C. Calder, D. A. Chamulak, E. F. Brown, and F. X. Timmes, Astrophys. J. , 2009, 701(2): 1582, arXiv: 0906.4384 [astro-ph.SR]
doi: 10.1088/0004-637X/701/2/1582
|
| 32 |
X. C. Meng and W. M. Yang, Astron. Astrophys. , 2011, 531: A94, arXiv: 1105.2860 [astro-ph.SR]
doi: 10.1051/0004-6361/201016325
|
| 33 |
A. G. Riess, A. V. Filippenko, P. Challis, A. Clocchiatti, , Astronom. J. , 1998, 116: 1009, arXiv: astroph/9805201
|
| 34 |
S. Perlmutter, G. Aldering, G. Goldhaber, R. A. Knop, , Astrophys. J. , 1999, 517: 565, arXiv: astro-ph/9812133
doi: 10.1086/307221
|
| 35 |
M. Sullivan, D. Le Borgne, C. J. Pritchet, A. Hodsman, , Astrophys. J. , 2006, 648(2): 868, arXiv: astroph/ 0605455
|
| 36 |
M. Sullivan, A. Conley, D. A. Howell, J. D. Neill, , Mon. Not. R. Astron. Soc. , 2010, 406: 782, arXiv: 1003.5119 [astro-ph.CO]
|
| 37 |
W. Li, R. Chornock, J. Leaman, A. V. Filippenko, D. Poznanski, X. Wang, M. Ganeshalingam, and F. Mannucci, Mon. Not. R. Astron. Soc. , 2011, 412(3): 1473, arXiv: 1006.4613 [astro-ph.SR]
doi: 10.1111/j.1365-2966.2011.18162.x
|
| 38 |
M. Hamuy, M. M. Phillips, N. B. Suntzeff, R. A. Schommer, J. Maza, and R. Avilé, Astron. J. , 1996, 112: 2398, arXiv: astro-ph/9609062
doi: 10.1086/118191
|
| 39 |
C. A. Tremonti, T. M. Heckman, G. Kauffmann, J. Brinchmann, S. Charlot, S. D. M. White, M. Seibert, E. W. Peng, D. J. Schlegel, A. Uomoto, M. Fukugita, and J. Brinkmann, Astrophys. J. , 2004, 613: 898, arXiv: astroph/0405537
|
| 40 |
J. S. Gallagher, P. M. Garnavich, P. Berlind, P. Challis, S. Jha, and R. P. Kirshner, Astrophys. J. , 2005, 634(1): 210, arXiv: astro-ph/0508180
doi: 10.1086/491664
|
| 41 |
J. S. Gallagher, P. M. Garnavich, N. Caldwell, R. P. Kirshner, S. W. Jha, W. Li, M. Ganeshalingam, and A. V. Filippenko, Astrophys. J. , 2008, 685(2): 752, arXiv: 0805.4360
doi: 10.1086/590659
|
| 42 |
J. D. Neill, M. Sullivan, D. A. Howell, A. Conley, , Astrophys. J. , 2009, 707(2): 1449, arXiv: 0911.0690
|
| 43 |
D. A. Howell, M. Sullivan, E. F. Brown, A. Conley, , Astrophys. J. , 2009, 691(1): 661, arXiv: 0810.0031
|
| 44 |
D. R. Silva and R. Elston, Astrophys. J. , 1994, 428: 511
doi: 10.1086/174263
|
| 45 |
G. Worthey, Astrophys. J. Suppl. , 1994, 95: 107
doi: 10.1086/192096
|
| 46 |
J. Guy, P. Astier, S. Nobili, N. Regnault, and R. Pain, Astron. Astrophys. , 2005, 443(3): 781, arXiv: astroph/ 0506583
|
| 47 |
J. Guy, P. Astier, S. Baumont, D. Hardin, , Astron. Astrophys. , 2007, 466(1): 11, arXiv: astro-ph/0701828
|
| 48 |
S. Jha, Exploding Stars, Near and Far, Ph.D. thesis, Harvard University , 2002
|
| 49 |
S. Jha, A. G. Riess, and R. P. Kirshner, Astrophys. J. , 2007, 659(1): 122, arXiv: astro-ph/0612666
doi: 10.1086/512054
|
| 50 |
C. R. Burns, M. Stritzinger, M. M. Phillips, S. Kattner, , Astronom. J. , 2011, 141: 19, arXiv: 1010.4040 [astroph. CO]
|
| 51 |
F. X. Timmes, E. F. Brown, and J. W. Truran, Astrophys. J. , 2003, 590(2): L83, arXiv: astro-ph/0305114
doi: 10.1086/376721
|
| 52 |
K. Nomoto, F. K. Thielemann, and K. Yokoi, Astrophys. J. , 1984, 286: 644
doi: 10.1086/162639
|
| 53 |
F. Mannucci, M. Della Valle, and N. Panagia, Mon. Not. R. Astron. Soc. , 2006, 370: 773, arXiv: astro-ph/0510315
doi: 10.1111/j.1365-2966.2006.10501.x
|
| 54 |
C. Raskin, E. Scannapieco, J. Rhoads, and M. D. Valle, Astrophys. J. , 2009, 707(1): 74, arXiv: 0909.4293
doi: 10.1088/0004-637X/707/1/74
|
| 55 |
T. D. Brandt, R. Tojeiro, E. Aubourg, A. Heavens, R. Jimenez, and M. A. Strauss, Astronom. J. , 2010, 140: 804, arXiv: 1002.0848 [astro-ph.GA]
|
| 56 |
N. Chotard, E. Gangler, G. Aldering, P. Antilogus, , Astron. Astrophys. , 2011, 529: L4, arXiv: 1103.5300 [astroph. CO]
doi: 10.1051/0004-6361/201116723
|
| 57 |
D. A. Howell, M. Sullivan, P. E. Nugent, R. S. Ellis, , Nature , 2006, 443: 308, arXiv: astroph/0609616
|
| 58 |
R. A. Scalzo, G. Aldering, P. Antilogus, C. Aragon, , Astrophys. J. , 2010, 713(2): 1073, arXiv: 1003.2217 [astroph. CO]
doi: 10.1088/0004-637X/713/2/1073
|
| 59 |
F. Yuan, R. M. Quimby, J. C. Wheeler, J. Vinkó, E. Chatzopoulos, C. W. Akerlof, S. Kulkarni, J. M. Miller, T. A. McKay, and F. Aharonian, Astrophys. J. , 2010, 715(2): 1338, arXiv: 1004.3329 [astro-ph.CO]
doi: 10.1088/0004-637X/715/2/1338
|
| 60 |
M. Tanaka, K. S. Kawabata, M. Yamanaka, K. Maeda, T. Hattori, K. Aoki, K. Nomoto, M. Iye, T. Sasaki, P. A.Mazzali, and E. Pian, Astrophys. J. , 2010, 714(2): 1209, arXiv: 0908.2057 [astro-ph.CO]
doi: 10.1088/0004-637X/714/2/1209
|
| 61 |
S. Chandrasekhar, Astrophys. J. , 1931, 74: 81
doi: 10.1086/143324
|
| 62 |
S. Chandrasekhar, Mon. Not. R. Astron. Soc. , 1935, 95: 207
|
| 63 |
S. Chandrasekhar, An introduction to the Study of Stellar Structure , New York: Dover, 1967
|
| 64 |
E. M?rtsell, L. Bergstr?m, and A. Goobar, Phys. Rev. D , 2002, 66(4): 047702, arXiv: astro-ph/0202153
doi: 10.1103/PhysRevD.66.047702
|
| 65 |
P. L. Biermann and L. Clavelli, Phys. Rev. D , 2011, 84(2): 023001, arXiv: 1011.1687 [astro-ph.HE]
doi: 10.1103/PhysRevD.84.023001
|
| 66 |
M. Livio, in: Type Ia Supernovae, Theory and Cosmology, edited by J. C. Niemeyer and J. W. Truran , 2000: 33
|
| 67 |
B. Wang and Z. Han, New Astron. Rev. , 2012, 56(4): 122, arXiv: 1204.1155 [astro-ph.SR]
doi: 10.1016/j.newar.2012.04.001
|
| 68 |
D. Branch, A. Fisher, and P. Nugent, Astron. J. , 1993, 106: 2383
doi: 10.1086/116810
|
| 69 |
M. Stritzinger, P. A. Mazzali, J. Sollerman, and S. Benetti, Astron. Astrophys. , 2006, 460: 793, arXiv: astroph/0609232
|
| 70 |
W. Li, J. Leaman, R. Chornock, A. V. Filippenko, D. Poznanski, M. Ganeshalingam, X. Wang, M. Modjaz, S. Jha, R. J. Foley, and N. Smith, Mon. Not. R. Astron. Soc. , 2011, 412(3): 1441, arXiv: 1006.4612 [astro-ph.SR]
doi: 10.1111/j.1365-2966.2011.18160.x
|
| 71 |
R. J. Foley, P. J. Challis, R. Chornock, M. Ganeshalingam, , arXiv: 1212.2209 [astro-ph.SR], 2012
|
| 72 |
E. Müler, in: Late Stages of Stellar Evolution. Computational Methods in Astrophysical Hydrodynamics, Lecture Notes in Physics, Vol. 373, edited by C. B. De Loore , Berlin: Springer-Verlag, 1991: 97
doi: 10.1007/BFb0032277
|
| 73 |
L. R. Yungelson and M. Livio, Astrophys. J. , 2000, 528(1): 108, arXiv: astro-ph/9907359
doi: 10.1086/308174
|
| 74 |
B. Wang, X. D. Li, and Z. W. Han, Mon. Not. R. Astron. Soc. , 2010, 401(4): 2729, arXiv: 0910.2138 [astro-ph.SR]
doi: 10.1111/j.1365-2966.2009.15857.x
|
| 75 |
A. J. Ruiter, K. Belczynski, and C. Fryer, Astrophys. J. , 2009, 699(2): 2026, arXiv: 0904.3108 [astro-ph.SR]
doi: 10.1088/0004-637X/699/2/2026
|
| 76 |
A. J. Ruiter, K. Belczynski, S. A. Sim, W. Hillebrandt, C. L. Fryer, M. Fink, and M. Kromer, Mon. Not. R. Astron. Soc. , 2011, 417(1): 408, arXiv: 1011.1407 [astro-ph.SR]
doi: 10.1111/j.1365-2966.2011.19276.x
|
| 77 |
E. Bravo, L. Piersanti, I. Domíguez, O. Straniero, J. Isern, and J. A. Escartin, Astron. Astrophys. , 2011, 535: A114, arXiv: 1110.1949 [astro-ph.SR]
doi: 10.1051/0004-6361/201117814
|
| 78 |
J. Whelan and I. Iben, Jr., Astrophys. J. , 1973, 186: 1007
doi: 10.1086/152565
|
| 79 |
I. Hachisu, M. Kato, and K. Nomoto, Astrophys. J. , 1996, 470(2): L97
doi: 10.1086/310303
|
| 80 |
Z. Han and P. Podsiadlowski, Mon. Not. R. Astron. Soc. , 2004, 350(4): 1301, arXiv: astro-ph/0309618
doi: 10.1111/j.1365-2966.2004.07713.x
|
| 81 |
B. Wang and Z.W. Han, Res. Astron. Astrophys. , 2010, 10: 235, arXiv: 1003.4568 [astroph.SR]
|
| 82 |
B. Wang, X. Meng, X. Chen, and Z. Han, Mon. Not. R. Astron. Soc. , 2009, 395(2): 847, arXiv: 0901.3496 [astroph. SR]
doi: 10.1111/j.1365-2966.2009.14545.x
|
| 83 |
D. Kasen, Astrophys. J. , 2010, 708(2): 1025, arXiv: 0909.0275 [astro-ph.HE]
|
| 84 |
P. E. Nugent, M. Sullivan, S. B. Cenko, R. C. Thomas, , Nature , 2011, 480(7377): 344, arXiv: 1110.6201 [astroph. CO]
|
| 85 |
P. J. Brown, K. S. Dawson, M. de Pasquale, C. Gronwall, S. Holland, S. Immler, P. Kuin, P. Mazzali, P. Milne, S. Oates, and M. Siegel, Astrophys. J. , 2012, 753(1): 22, arXiv: 1110.2538 [astro-ph.CO]
doi: 10.1088/0004-637X/753/1/22
|
| 86 |
W. Li, J. S. Bloom, P. Podsiadlowski, A. A. Miller, , Nature , 2011, 480(7377): 348, arXiv: 1109.1593 [astro-ph.CO]
doi: 10.1038/nature10646
|
| 87 |
J. C. Wheeler, Astrophys. J. , 2012, 758(2): 123, arXiv: 1209.1021 [astro-ph.SR]
doi: 10.1088/0004-637X/758/2/123
|
| 88 |
B. Dilday, D. A. Howell, S. B. Cenko, J. M. Silverman, , Science , 2012, 337(6097): 942, arXiv: 1207.1306 [astroph. CO]
|
| 89 |
P. A. Mazzali, D. N. Sauer, A. Pastorello, S. Benetti, and W. Hillebrandt, Mon. Not. R. Astron. Soc. , 2008, 386(4): 1897, arXiv: 0803.1383
doi: 10.1111/j.1365-2966.2008.13199.x
|
| 90 |
W. D. Arnett, Astrophys. Space Sci. , 1969, 5(2): 180
doi: 10.1007/BF00650291
|
| 91 |
F. K. R?pke, W. Hillebrandt, W. Schmidt, J. C. Niemeyer, S. I. Blinnikov, and P. A. Mazzali, Astrophys. J. , 2007, 668(2): 1132, arXiv: 0707.1024
doi: 10.1086/521347
|
| 92 |
A. M. Khokhlov, Astron. Astrophys. , 1991, 245: 114
|
| 93 |
P. H?flich, A. M. Khokhlov, and J. C. Wheeler, Astrophys. J. , 1995, 444: 831
doi: 10.1086/175656
|
| 94 |
P. H?flich and A. Khokhlov, Astrophys. J. , 1996, 457: 500, arXiv: astro-ph/9602025
doi: 10.1086/176748
|
| 95 |
D. Arnett and E. Livne, Astrophys. J. , 1994, 427: 315
doi: 10.1086/174142
|
| 96 |
D. Arnett and E. Livne, Astrophys. J. , 1994, 427: 330
doi: 10.1086/174143
|
| 97 |
T. Plewa, A. C. Calder, and D. Q. Lamb, Astrophys. J. , 2004, 612(1): L37
doi: 10.1086/424036
|
| 98 |
G. C. IV Jordan, R. T. Fisher, D. M. Townsley, A. C. Calder, C. Graziani, S. Asida, D. Q. Lamb, and J. W. Truran, Astrophys. J. , 2008, 681(2): 1448, arXiv: astro-ph/0703573
|
| 99 |
I. R. Seitenzahl, C. A. Meakin, D. Q. Lamb, and J. W. Truran, Astrophys. J. , 2009, 700(1): 642, arXiv: 0905.3104 [astro-ph.SR]
doi: 10.1088/0004-637X/700/1/642
|
| 100 |
D. A. Chamulak, C. A. Meakin, I. R. Seitenzahl, and J. W. Truran, Astrophys. J. , 2012, 744(1): 27, arXiv: 1103.3062 [astro-ph.SR]
doi: 10.1088/0004-637X/744/1/27
|
| 101 |
S. I. Blinnikov and A.M. Khokhlov, Sov. Astron. Lett. , 1986, 12: 131
|
| 102 |
S. E. Woosley, in: Supernovae, edited by A. G. Petschek , 1990: 182
doi: 10.1007/978-1-4612-3286-5_8
|
| 103 |
A. M. Khokhlov, E. S. Oran, and J. C. Wheeler, Astrophys. J. , 1997, 478(2): 678, arXiv: astro-ph/9612226
doi: 10.1086/303815
|
| 104 |
J. C. Niemeyer and S. E. Woosley, Astrophys. J. , 1997, 475(2): 740, arXiv: astro-ph/9607032
doi: 10.1086/303544
|
| 105 |
P. H?flich, J. C. Wheeler, and F. K. Thielemann, Astrophys. J. , 1998, 495: 617, arXiv: astro-ph/9709233
doi: 10.1086/305327
|
| 106 |
J. C. Niemeyer, Astrophys. J. , 1999, 523(1): L57, arXiv: astro-ph/9906142
|
| 107 |
K. Maeda, S. Benetti, M. Stritzinger, F. K. R?pke, G. Folatelli, J. Sollerman, S. Taubenberger, K. Nomoto, G. Leloudas, M. Hamuy, M. Tanaka, P. A. Mazzali, and N. Elias-Rosa, Nature , 2010, 466(7302): 82, arXiv: 1006.5888 [astro-ph.CO]
doi: 10.1038/nature09122
|
| 108 |
A. V. Tutukov and L. R. Iungelson, Astrofizika , 1976, 12: 521
|
| 109 |
A. V. Tutukov and L. R. Yungelson, Acta Astronaut. , 1979, 29: 665
|
| 110 |
R. F. Webbink, Astrophys. J. , 1984, 277: 355
doi: 10.1086/161701
|
| 111 |
I. Iben, Jr. and A. V. Tutukov, Astrophys. J. Suppl. , 1984, 54: 335
|
| 112 |
H. Saio and K. Nomoto, Astron. Astrophys. , 1985, 150: L21
|
| 113 |
H. Saio and K. Nomoto, Astrophys. J. , 2004, 615(1): 444, arXiv: astro-ph/0401141
doi: 10.1086/423976
|
| 114 |
K. Nomoto and Y. Kondo, Astrophys. J. , 1991, 367: L19
doi: 10.1086/185922
|
| 115 |
Y. Kawai, H. Saio, and K. Nomoto, Astrophys. J. , 1987, 315: 229
doi: 10.1086/165126
|
| 116 |
R. Pakmor, S. Hachinger, F. K. R?pke, and W. Hillebrandt, Astron. Astrophys. , 2011, 528: A117, arXiv: 1102.1354 [astroph. SR]
doi: 10.1051/0004-6361/201015653
|
| 117 |
S. Rosswog, D. Kasen, J. Guillochon, and E. Ramirez-Ruiz, Astrophys. J. , 2009, 705(2): L128, arXiv: 0907.3196 [astroph. HE]
doi: 10.1088/0004-637X/705/2/L128
|
| 118 |
C. Raskin, F. X. Timmes, E. Scannapieco, S. Diehl, and C. Fryer, Mon. Not. R. Astron. Soc. , 2009, 399(1): L156, arXiv: 0907.3915 [astro-ph.SR]
doi: 10.1111/j.1745-3933.2009.00743.x
|
| 119 |
C. Raskin, E. Scannapieco, G. Rockefeller, C. Fryer, S. Diehl, and F. X. Timmes, Astrophys. J. , 2010, 724(1): 111, arXiv: 1009.2507 [astro-ph.SR]
doi: 10.1088/0004-637X/724/1/111
|
| 120 |
P. Loré-Aguilar, J. Isern, and E. Garcí-Berro, Mon. Not. R. Astron. Soc. , 2010, 406(4): 2749, arXiv: 1004.4783 [astroph. SR]
doi: 10.1111/j.1365-2966.2010.16878.x
|
| 121 |
X. Meng and W. Yang, Astron. Astrophys. , 2012, 543: A137, arXiv: 1205.2452 [astro-ph.SR]
doi: 10.1051/0004-6361/201218810
|
| 122 |
W. Benz, A. G.W. Cameron, W. H. Press, and R. L. Bowers, Astrophys. J. , 1990, 348: 647
doi: 10.1086/168273
|
| 123 |
S. C. Yoon, P. Podsiadlowski, and S. Rosswog, Mon. Not. R. Astron. Soc. , 2007, 380(3): 933, arXiv: 0704.0297
doi: 10.1111/j.1365-2966.2007.12161.x
|
| 124 |
P. Loré-Aguilar, J. Isern, and E. Garcí-Berro, Astron. Astrophys. , 2009, 500(3): 1193
doi: 10.1051/0004-6361/200811060
|
| 125 |
K. J. Shen, L. Bildsten, D. Kasen, and E. Quataert, Astrophys. J. , 2012, 748(1): 35
doi: 10.1088/0004-637X/748/1/35
|
| 126 |
C. L. Fryer and S. Diehl, in: Hydrogen-Deficient Stars, Astronomical Society of the Pacific Conference Series, Vol. 391, edited by A. Werner and T. Rauch , 2008: 335, arXiv: 0711.0864
|
| 127 |
S. Diehl, C. Fryer, A. Hungerford, G. Rockefeller, M. E. Bennet, F. Herwig, R. Hirschi, M. Pignatari, G. Magkotsios, F. X. Timmes, P. Young, G. C. Clayton, P. Motl, and J. E. Tohline, in: Nuclei in the Cosmos (NIC X) , 2008
|
| 128 |
M. C. R. D’Souza, P. M. Motl, J. E. Tohline, and J. Frank, Astrophys. J. , 2006, 643: 381, arXiv: astroph/0512137
|
| 129 |
P. M. Motl, J. Frank, J. E. Tohline, and M. C. R. D’Souza, Astrophys. J. , 2007, 670: 1314, arXiv: astroph/0702388
|
| 130 |
M. Dan, S. Rosswog, J. Guillochon, and E. Ramirez-Ruiz, Astrophys. J. , 2011, 737(2): 89, arXiv: 1101.5132 [astroph. HE]
doi: 10.1088/0004-637X/737/2/89
|
| 131 |
M. Dan, S. Rosswog, J. Guillochon, and E. Ramirez-Ruiz, Mon. Not. R. Astron. Soc. , 2012, 422(3): 2417, arXiv: 1201.2406 [astro-ph.HE]
doi: 10.1111/j.1365-2966.2012.20794.x
|
| 132 |
R. Pakmor, P. Edelmann, F. K. Roepke, and W. Hillebrandt, arXiv: 1205.5806 [astroph.HE], 2012
|
| 133 |
R. Pakmor, M. Kromer, F. K. R?pke, S. A. Sim, A. J. Ruiter, and W. Hillebrandt, Nature , 2010, 463(7277): 61, arXiv: 0911.0926 [astro-ph.HE]
doi: 10.1038/nature08642
|
| 134 |
R. Pakmor, M. Kromer, S. Taubenberger, S. A. Sim, F. K. R?pke, and W. Hillebrandt, Astrophys. J. , 2012, 747(1): L10, arXiv: 1201.5123 [astro-ph.HE]
doi: 10.1088/2041-8205/747/1/L10
|
| 135 |
M. Steinmetz, E. Muller, and W. Hillebrandt, Astron. Astrophys. , 1992, 254: 177
|
| 136 |
J. M. M. Pfannes, J. C. Niemeyer, W. Schmidt, and C. Klingenberg, Astron. Astrophys. , 2010, 509: A74, arXiv: 0911.3540 [astro-ph.HE]
doi: 10.1051/0004-6361/200912032
|
| 137 |
J. M. M. Pfannes, J. C. Niemeyer, and W. Schmidt, Astron. Astrophys. , 2010, 509: A75, arXiv: 0911.3545 [astro-ph.HE]
doi: 10.1051/0004-6361/200912033
|
| 138 |
I. Hachisu, M. Kato, H. Saio, and K. Nomoto, Astrophys. J. , 2012, 744(1): 69, arXiv: 1106.3510 [astro-ph.SR]
doi: 10.1088/0004-637X/744/1/69
|
| 139 |
S. E. Woosley, T. A. Weaver, and R. E. Taam, in: Texas Workshop on Type I Supernovae, edited by J. C. Wheeler , 1980: 96
|
| 140 |
R. E. Taam, Astrophys. J. , 1980, 237: 142
doi: 10.1086/157852
|
| 141 |
R. E. Taam, Astrophys. J. , 1980, 242: 749
doi: 10.1086/158509
|
| 142 |
K. Nomoto, Space Sci. Rev. , 1980, 27(3-4): 563
|
| 143 |
K. Nomoto, Astrophys. J. , 1982, 257: 780
|
| 144 |
E. Livne, Astrophys. J. , 1990, 354: L53
|
| 145 |
S. E. Woosley and T. A. Weaver, Astrophys. J. , 1994, 423: 371
doi: 10.1086/173813
|
| 146 |
E. Livne and A. S. Glasner, Astrophys. J. , 1991, 370: 272
doi: 10.1086/169813
|
| 147 |
E. Livne and D. Arnett, Astrophys. J. , 1995, 452: 62
doi: 10.1086/176279
|
| 148 |
P. Hoeflich, A. Khokhlov, J. C. Wheeler, M. M. Phillips, N. B. Suntzeff, and M. Hamuy, Astrophys. J. , 1996, 472: L81, arXiv: astro-ph/9609070
|
| 149 |
D. J. R. Wiggins and S. A. E. G. Falle, Mon. Not. R. Astron. Soc. , 1997, 287: 575
doi: 10.1093/mnras/287.3.575
|
| 150 |
D. J. R. Wiggins, G. J. Sharpe, and S. A. E. G. Falle, Mon. Not. R. Astron. Soc. , 1998, 301(2): 405
doi: 10.1046/j.1365-8711.1998.02007.x
|
| 151 |
D. Garcí-Senz, E. Bravo, and S. E. Woosley, Astron. Astrophys. , 1999, 349: 177
|
| 152 |
M. Fink, W. Hillebrandt, and F. K. R?pke, Astron. Astrophys. , 2007, 476(3): 1133, arXiv: 0710.5486
doi: 10.1051/0004-6361:20078438
|
| 153 |
S. A. Sim, F. K. R?pke, W. Hillebrandt, M. Kromer, R. Pakmor, M. Fink, A. J. Ruiter, and I. R. Seitenzahl, Astrophys. J. , 2010, 714(1): L52, arXiv: 1003.2917 [astro-ph.HE]
doi: 10.1088/2041-8205/714/1/L52
|
| 154 |
L. Bildsten, K. J. Shen, N. N. Weinberg, and G. Nelemans, Astrophys. J. Lett. , 2007, 662: L95, arXiv: astroph/0703578
|
| 155 |
M. Fink, F. K. R?pke, W. Hillebrandt, I. R. Seitenzahl, S. A. Sim, and M. Kromer, Astron. Astrophys. , 2010, 514: A53, arXiv: 1002.2173 [astro-ph.SR]
doi: 10.1051/0004-6361/200913892
|
| 156 |
M. Kromer, S. A. Sim, M. Fink, F. K. R?pke, I. R. Seitenzahl, and W. Hillebrandt, Astrophys. J. , 2010, 719(2): 1067, arXiv: 1006.4489 [astro-ph.HE]
doi: 10.1088/0004-637X/719/2/1067
|
| 157 |
S. E. Woosley and D. Kasen, Astrophys. J. , 2011, 734(1): 38, arXiv: 1010.5292 [astro-ph.HE]
doi: 10.1088/0004-637X/734/1/38
|
| 158 |
S. A. Sim, M. Fink, M. Kromer, F. K. R?pke, A. J. Ruiter, and W. Hillebrandt, Mon. Not. R. Astron. Soc. , 2012, 420(4): 3003, arXiv: 1111.2117 [astro-ph.HE]
doi: 10.1111/j.1365-2966.2011.20162.x
|
| 159 |
K. Nomoto, Astrophys. J. , 1982, 253: 798
|
| 160 |
S. E. Woosley and T. A. Weaver, Annu. Rev. Astron. Astrophys. , 1986, 24(1): 205
doi: 10.1146/annurev.aa.24.090186.001225
|
| 161 |
A. Nonaka, A. J. Aspden, M. Zingale, A. S. Almgren, J. B. Bell, and S. E. Woosley, Astrophys. J. , 2012, 745(1): 73, arXiv: 1111.3086 [astro-ph.HE]
doi: 10.1088/0004-637X/745/1/73
|
| 162 |
A. L. Piro and L. Bildsten, Astrophys. J. , 2008, 673(2): 1009, arXiv: 0710.1600
doi: 10.1086/524189
|
| 163 |
F. K. R?pke, Astrophys. J. , 2007, 668(2): 1103, arXiv: 0709.4095
doi: 10.1086/520830
|
| 164 |
I. R. Seitenzahl, C. A. Meakin, D. M. Townsley, D. Q. Lamb, and J. W. Truran, Astrophys. J. , 2009, 696(1): 515, arXiv: 0901.3677
doi: 10.1088/0004-637X/696/1/515
|
| 165 |
S. E. Woosley, A. R. Kerstein, V. Sankaran, A. J. Aspden, and F. K. R?pke, Astrophys. J. , 2009, 704(1): 25, arXiv: 0811.3610
doi: 10.1088/0004-637X/704/1/255
|
| 166 |
W. Schmidt, F. Ciaraldi-Schoolmann, J. C. Niemeyer, F. K. R?pke, and W. Hillebrandt, Astrophys. J. , 2010, 710(2): 1683, arXiv: 0911.4345
doi: 10.1088/0004-637X/710/2/1683
|
| 167 |
A. Y. Poludnenko, T. A. Gardiner, and E. S. Oran, Phys. Rev. Lett. , 2011, 107(5): 054501, arXiv: 1106.3696 [astroph. HE]
doi: 10.1103/PhysRevLett.107.054501
|
| 168 |
C. Charignon and J. P. Chièze, arXiv: 1301.1523 [astroph. HE], 2013
|
| 169 |
S. B. Pope, Ann. Rev. Fluid Mech. , 1987, 19(1): 237
doi: 10.1146/annurev.fl.19.010187.001321
|
| 170 |
I. Golombek and J. C. Niemeyer, Astron. Astrophys. , 2005, 438(2): 611, arXiv: astro-ph/0503617
doi: 10.1051/0004-6361:20042402
|
| 171 |
F. K. R?pke and W. Hillebrandt, Astron. Astrophys. , 2005, 429: L29, arXiv: astro-ph/0411667
doi: 10.1051/0004-6361:200400100
|
| 172 |
A. J. Aspden, J. B. Bell, M. S. Day, S. E. Woosley, and M. Zingale, Astrophys. J. , 2008, 689(2): 1173, arXiv: 0811.2816
doi: 10.1086/592726
|
| 173 |
A. J. Aspden, J. B. Bell, and S. E. Woosley, Astrophys. J. , 2010, 710(2): 1654
doi: 10.1088/0004-637X/710/2/1654
|
| 174 |
A. Y. Poludnenko and E. S. Oran, Combust. Flame , 2011, 157(5): 995
doi: 10.1016/j.combustflame.2009.11.018
|
| 175 |
A. Y. Poludnenko and E. S. Oran, Combust. Flame , 2011, 158(2): 301
doi: 10.1016/j.combustflame.2010.09.002
|
| 176 |
S. E. Woosley, Astrophys. J. , 2007, 668(2): 1109, arXiv: 0709.4237
doi: 10.1086/520835
|
| 177 |
A. M. Lisewski, W. Hillebrandt, and S. E. Woosley, Astrophys. J. , 2000, 538(2): 831, arXiv: astro-ph/9910056
doi: 10.1086/309158
|
| 178 |
F. K. R?pke and J. C. Niemeyer, Astron. Astrophys. , 2007, 464(2): 683, arXiv: astro-ph/0703378
doi: 10.1051/0004-6361:20066585
|
| 179 |
E. Bravo and D. García-Senz, Astron. Astrophys. , 2008, 478(3): 843, arXiv: 0712.0510
doi: 10.1051/0004-6361:20078424
|
| 180 |
K. Maeda, F. K. R?pke, M. Fink, W. Hillebrandt, C. Travaglio, and F. K. Thielemann, Astrophys. J. , 2010, 712(1): 624, arXiv: 1002.2153 [astro-ph.SR]
doi: 10.1088/0004-637X/712/1/624
|
| 181 |
A. P. Jackson, A. C. Calder, D. M. Townsley, D. A. Chamulak, E. F. Brown, and F. X. Timmes, Astrophys. J. , 2010, 720(1): 99, arXiv: 1007.1138 [astro-ph.SR]
doi: 10.1088/0004-637X/720/1/99
|
| 182 |
O. Straniero, I. Domínguez, G. Imbriani, and L. Piersanti, Astrophys. J. , 2003, 583: 878, arXiv: astroph/0210191
|
| 183 |
H. Umeda, K. Nomoto, H. Yamaoka, and S. Wanajo, Astrophys. J. , 1999, 513(2): 861
doi: 10.1086/306887
|
| 184 |
D. A. Chamulak, E. F. Brown, F. X. Timmes, and K. Dupczak, Astrophys. J. , 2008, 677(1): 160
doi: 10.1086/528944
|
| 185 |
D. Branch, M. Livio, L. R. Yungelson, F. R. Boffi, and E. Baron, Publ. Astron. Soc. Pac. , 1995, 107: 1019
doi: 10.1086/133657
|
| 186 |
L. R. Gasques, A. V. Afanasjev, E. F. Aguilera, M. Beard, L. C. Chamon, P. Ring, M. Wiescher, and D. G. Yakovlev, Phys. Rev. C , 2005, 72: 025806, arXiv: astroph/0506386
|
| 187 |
D. G. Yakovlev, L. R. Gasques, A. V. Afanasjev, M. Beard, and M. Wiescher, Phys. Rev. C , 2006, 74(3): 035803, arXiv: astro-ph/0608488
doi: 10.1103/PhysRevC.74.035803
|
| 188 |
A. C. Calder, D. M. Townsley, I. R. Seitenzahl, F. Peng, O. E. B. Messer, N. Vladimirova, E. F. Brown, J. W. Truran, and D. Q. Lamb, Astrophys. J. , 2007, 656(1): 313, arXiv: astro-ph/0611009
doi: 10.1086/510709
|
| 189 |
F. X. Timmes and S. E. Woosley, Astrophys. J. , 1992, 396: 649
doi: 10.1086/171746
|
| 190 |
D. A. Chamulak, E. F. Brown, and F. X. Timmes, Astrophys. J. , 2007, 655(2): L93, arXiv: astro-ph/0612507
doi: 10.1086/511856
|
| 191 |
J. C. Niemeyer and W. Hillebrandt, Astrophys. J. , 1995, 452: 769
doi: 10.1086/176345
|
| 192 |
M. Zingale and L. J. Dursi, Astrophys. J. , 2007, 656(1): 333, arXiv: astro-ph/0610297
doi: 10.1086/510306
|
| 193 |
E. Bravo, J. Isern, R. Canal, and J. Labay, Astron. Astrophys. , 1992, 257: 534
|
| 194 |
L. G. Althaus, E. García-Berro, I. Renedo, J. Isern, A. H. Córsico, and R. D. Rohrmann, Astrophys. J. , 2010, 719(1): 612, arXiv: 1006.4170 [astro-ph.SR]
doi: 10.1088/0004-637X/719/1/612
|
| 195 |
E. Bravo, L. G. Althaus, E. García-Berro, and I. Domínguez, Astron. Astrophys. , 2011, 526: A26, arXiv: 1010.5098 [astro-ph.SR]
doi: 10.1051/0004-6361/201015506
|
| 196 |
D. Kasen, F. K. R?pke, and S. E. Woosley, Nature , 2009, 460(7257): 869, arXiv: 0907.0708 [astroph.HE]
doi: 10.1038/nature08256
|
| 197 |
P. H?flich, J. C. Wheeler, and F. K. Thielemann, Astrophys. J. , 1998, 495(2): 617, arXiv: astro-ph/9709233
doi: 10.1086/305327
|
| 198 |
H. Umeda, K. Nomoto, C. Kobayashi, I. Hachisu, and M. Kato, Astrophys. J. , 1999, 522(1): L43
doi: 10.1086/312213
|
| 199 |
F. K. R?pke and W. Hillebrandt, Astron. Astrophys. , 2004, 420: L1, arXiv: astro-ph/0403509
doi: 10.1051/0004-6361:20040135
|
| 200 |
E. Bravo, I. Domínguez, C. Badenes, L. Piersanti, and O. Straniero, Astrophys. J. , 2010, 711(2): L66 arXiv: 1002.0681
doi: 10.1088/2041-8205/711/2/L66
|
| 201 |
C. Contreras, M. Hamuy, M. M. Phillips, G. Folatelli, , Astronom. J. , 2010, 139: 519, arXiv: 0910.3330 [astroph. CO]
|
| 202 |
G. Folatelli, M. M. Phillips, C. R. Burns, C. Contreras, , Astronom. J. , 2010, 139: 120, arXiv: 0910.3317 [astroph. CO]
|
| 203 |
P. H?flich and J. Stein, Astrophys. J. , 2002, 568(2): 779, arXiv: astro-ph/0104226
doi: 10.1086/338981
|
| 204 |
S. E. Woosley, S. Wunsch, and M. Kuhlen, Astrophys. J. , 2004, 607(2): 921, arXiv: astro-ph/0307565
doi: 10.1086/383530
|
| 205 |
M. Kuhlen, S. E.Woosley, and G. A. Glatzmaier, Astrophys. J. , 2006, 640(1): 407, arXiv: astro-ph/0509367
doi: 10.1086/500105
|
| 206 |
A. L. Piro and P. Chang, Astrophys. J. , 2008, 678(2): 1158, arXiv: 0801.1321
doi: 10.1086/529368
|
| 207 |
M. Zingale, A. S. Almgren, J. B. Bell, A. Nonaka, and S. E. Woosley, Astrophys. J. , 2009, 704(1): 196, arXiv: 0908.2668
doi: 10.1088/0004-637X/704/1/196
|
| 208 |
M. Zingale, A. Nonaka, A. S. Almgren, J. B. Bell, C. M. Malone, and S. E. Woosley, Astrophys. J. , 2011, 740(1): 8
doi: 10.1088/0004-637X/740/1/8
|
| 209 |
C. L. Jiang, K. E. Rehm, B. B. Back, and R. V. F. Janssens, Phys. Rev. C , 2007, 75(1): 015803
doi: 10.1103/PhysRevC.75.015803
|
| 210 |
R. L. Cooper, A. W. Steiner, and E. F. Brown, Astrophys. J. , 2009, 702(1): 660, arXiv: 0903.3994 [astroph.HE]
doi: 10.1088/0004-637X/702/1/660
|
| 211 |
L. Iapichino and P. Lesaffre, Astron. Astrophys. , 2010, 512: A27, arXiv: 1001.2165 [astro-ph.SR]
doi: 10.1051/0004-6361/200913306
|
| 212 |
B. Paczyński, Astrophys. Lett. , 1972, 11: 53
|
| 213 |
I. Iben, Jr., Astrophys. J. , 1978, 219: 213
doi: 10.1086/155769
|
| 214 |
I. Iben, Jr., Astrophys. J. , 1978, 226: 996
doi: 10.1086/156680
|
| 215 |
I. Iben, Jr., Astrophys. J. , 1982, 253: 248
doi: 10.1086/159630
|
| 216 |
J. Stein, Z. Barkat, and J. C. Wheeler, Astrophys. J. , 1999, 523(1): 381
doi: 10.1086/307715
|
| 217 |
P. Lesaffre, P. Podsiadlowski, and C. A. Tout, Mon. Not. R. Astron. Soc. , 2005, 356(1): 131
doi: 10.1111/j.1365-2966.2004.08428.x
|
| 218 |
E. Bravo, J. Isern, R. Canal, and J. Labay, Astrophys. Space Sci. , 1990, 169(1-2): 19
doi: 10.1007/BF00640679
|
| 219 |
R. Fisher, D. Falta, G. Jordan, and D. Lamb, in: Gravitation and Astrophysics, edited by J. Luo, Z.-B. Zhou, H.-C. Yeh, and J.-P. Hsu , 2010: 335–344 , arXiv: 1005.0026 [astroph. SR]
|
| 220 |
I. R. Seitenzahl, F. Ciaraldi-Schoolmann, F. K. R?pke, M. Fink, W. Hillebrandt, M. Kromer, R. Pakmor, A. J. Ruiter, S. A. Sim, and S. Taubenberger, Mon. Not. R. Astron. Soc. , 2013, 429(2): 1156, arXiv: 1211.3015 [astro-ph.SR]
doi: 10.1093/mnras/sts402
|
| 222 |
B. Fryxell, K. Olson, P. Ricker, F. X. Timmes, M. Zingale, D. Q. Lamb, P. MacNeice, R. Rosner, J. W. Truran, and H. Tufo, Astrophys. J. Suppl. , 2000, 131(1): 273
doi: 10.1086/317361
|
| 223 |
A. C. Calder, B. C. Curtis, L. J. Dursi, B. Fryxell, G. Henry, P. MacNeice, K. Olson, P. Ricker, R. Rosner, F. X. Timmes, H. M. Tufo, J. W. Truran, and M. Zingale, in: Proceedings of Supercomputing 2000 , 2000, http://sc2000.org
|
| 224 |
A. C. Calder, B. Fryxell, T. Plewa, R. Rosner, , Astrophys. J. Suppl. , 2002, 143(1): 201
doi: 10.1086/342267
|
| 225 |
E. F. Brown, A. C. Calder, T. Plewa, P. M. Ricker, K. Robinson, and J. B. Gallagher, Nucl. Phys. A. , 2005, 758: 451, arXiv: astro-ph/0505417
doi: 10.1016/j.nuclphysa.2005.05.083
|
| 226 |
D. M. Townsley, F. X. Timmes, A. P. Jackson, A. C. Calder, and E. F. Brown, Astrophys. J. , 2012 (to be submitted)
|
| 227 |
D. M. Townsley, A. C. Calder, S. M. Asida, I. R. Seitenzahl, F. Peng, N. Vladimirova, D. Q. Lamb, and J. W. Truran, Astrophys. J. , 2007, 668(2): 1118, arXiv: 0706.1094
doi: 10.1086/521013
|
| 228 |
A. M. Khokhlov, Astrophys. J. , 1995, 449: 695
doi: 10.1086/176091
|
| 229 |
N. Vladimirova, G. Weirs, and L. Ryzhik, Combust. Theory Modeling , 2006, 10(5): 727
doi: 10.1080/13647830500464146
|
| 230 |
F. X. Timmes and S. E. Woosley, Astrophys. J. , 1992, 396: 649
doi: 10.1086/171746
|
| 231 |
G. Taylor, Royal Society of London Proceedings Series A , 1950, 201(1065): 192
|
| 232 |
S. Chandrasekhar, Hydrodynamic and Hydromagnetic Stability , New York: Dover, 1981
|
| 233 |
D. Townsley, Comput. Sci. Eng. , 2009, 11(2): 18
doi: 10.1109/MCSE.2009.41
|
| 234 |
V. N. Gamezo, A.M. Khokhlov, E. S. Oran, A. Y. Chtchelkanova, and R. O. Rosenberg, Science , 2003, 299(5603): 77
doi: 10.1126/science.1078129
|
| 235 |
A. P. Jackson, D. M. Townsley, and A. C. Calder, 2012 (in preparation)
|
| 236 |
D. Bodansky, D. D. Clayton, and W. A. Fowler, Astrophys. J. Suppl. , 1968, 16: 299
doi: 10.1086/190176
|
| 237 |
S. E. Woosley, W. D. Arnett, and D. D. Clayton, Astrophys. J. Suppl. , 1973, 26: 231
doi: 10.1086/190282
|
| 238 |
V. S. Imshennik, S. S. Filippov, and A. M. Khokhlov, Sov. Astron. Lett. , 1981, 7: 121
|
| 239 |
A. M. Khokhlov, Sov. Astron. Lett. , 1981, 7: 410
|
| 240 |
A. M. Khokhlov, Sov. Astron. Lett. , 1983, 9: 160
|
| 241 |
K. Langanke and G. Martínez-Pinedo, At. Data Nucl. Data Tables , 2001, 79(1): 1
doi: 10.1006/adnd.2001.0865
|
| 242 |
I. R. Seitenzahl, D. M. Townsley, F. Peng, and J. W. Truran, At. Data Nucl. Data Tables , 2009, 95(1): 96
doi: 10.1016/j.adt.2008.08.001
|
| 243 |
C. A. Meakin, I. Seitenzahl, D. Townsley, G. C. Jordan, J. Truran, and D. Lamb, Astrophys. J. , 2009, 693(2): 1188, arXiv: 0806.4972
doi: 10.1088/0004-637X/693/2/1188
|
| 244 |
V. N. Gamezo, A. M. Khokhlov, and E. S. Oran, Astrophys. J. , 2005, 623(1): 337, arXiv: astro-ph/0409598
doi: 10.1086/428767
|
| 245 |
A. M. Khokhlov, arXiv: astroph/0008463, 2000
|
| 246 |
K. Konishi, D. Cinabro, P. M. Garnavich, Y. Ihara, R. Kessler, J. Marriner, D. P. Schneider, M. Smith, H. Spinka, J. C. Wheeler, and N. Yasuda, arXiv: 1101.4269 [astroph. CO], 2011
|
| 247 |
B. Carroll and D. Ostlie, An Introduction to Modern Astrophysics, Pearson Addison-Wesley , 2007
|
| 248 |
B. K. Krueger, A. P. Jackson, D. M. Townsley, A. C. Calder, E. F. Brown, and F. X. Timmes, Astrophys. J. Lett. , 2010, 719: L5, arXiv: 1007.0910
doi: 10.1088/2041-8205/719/1/L5
|
| 249 |
B. K. Krueger, A. P. Jackson, A. C. Calder, D. M. Townsley, E. F. Brown, and F. X. Timmes, Astrophys. J. , 2012, 757(2): 175
doi: 10.1088/0004-637X/757/2/175
|
| 250 |
G. Goldhaber, D. E. Groom, A. Kim, G. Aldering, , Astrophys. J. , 2001, 558: 359, arXiv: astroph/0104382
|
| 251 |
C. J. Hansen, S. D. Kawaler, and V. Trimble, Stellar interiors: Physical Principles, Structure, and Evolution , New York: Springer-Verlag, 2004
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