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Frontiers of Physics

ISSN 2095-0462

ISSN 2095-0470(Online)

CN 11-5994/O4

邮发代号 80-965

2019 Impact Factor: 2.502

Frontiers of Physics  2013, Vol. 8 Issue (6): 605-608   https://doi.org/10.1007/s11467-013-0351-7
  EDITORIAL 本期目录
Preface: High Energy Astrophysics
Preface: High Energy Astrophysics
Bing Zhang1,2(), Peter Mésáros3()
1. Kavli Institute for Astronomy and Astrophysics and Department of Astronomy, Peking University, China; 2. Department of Physics and Astronomy, University of Nevada, Las Vegas, USA; 3. Department of Astronomy and Astrophysics, Department of Physics, and Center for Particle and Gravitational Astrophysics, Pennsylvania State University, University Park, PA 16802, USA
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Abstract

High energy astrophysics is one of the most active branches in the contemporary astrophysics. It studies astrophysical objects that emit X-ray and γ-ray photons, such as accreting super-massive and stellar-size black holes, and various species of neutron stars. With the operations of many space-borne and ground-based observational facilities, high energy astrophysics has enjoyed rapid development in the past decades. It is foreseen that the field will continue to advance rapidly in the coming decade, with possible ground-breaking discoveries of astrophysical sources in the high-energy neutrino and gravitational wave channels. This Special Issue of Frontiers of Physics is dedicated to a systematic survey of the field of high energy astrophysics as it stands in 2013.

收稿日期: 2013-05-24      出版日期: 2013-12-01
Corresponding Author(s): Zhang Bing,Email:zhang@physics.unlv.edu; Mésáros Peter,Email:nnp@astro.psu.edu   
 引用本文:   
. Preface: High Energy Astrophysics[J]. Frontiers of Physics, 2013, 8(6): 605-608.
Bing Zhang, Peter Mésáros. Preface: High Energy Astrophysics. Front. Phys. , 2013, 8(6): 605-608.
 链接本文:  
https://academic.hep.com.cn/fop/CN/10.1007/s11467-013-0351-7
https://academic.hep.com.cn/fop/CN/Y2013/V8/I6/605
1 H. Krawczynski and E. Treister, Front. Phys. , 2013, 8(6): 609, arXiv: 1301.4179
2 S.-N. Zhang, Front. Phys. , 2013, 8(6): 630, arXiv: 1302.5485
3 N. Gehrels and S. Razzaque, Front. Phys. , 2013, 8(6): 661, arXiv: 1301.0840
4 A. K. Harding, Front. Phys. , 2013, 8(6): 679, arXiv: 1302.0869
5 S. Ritz, Front. Phys. , 2013, 8(6): 693
doi: 10.1007/s11467-013-0401-1
6 F. M. Rieger, E. de O?a-Wilhelmi, and F. A. Aharonian, Front. Phys. , 2013, 8(6): 714, arXiv: 1302.5603
7 T. K. Gaisser, T. Stanev, and S. Tilav, Front. Phys. , 2013, 8(6): 748, arXiv: 1303.3565
8 F. Halzen, Front. Phys. , 2013, 8(6): 759
doi: 10.1007/s11467-013-0299-7
9 G. González, A. Viceré, and L. Wen, Front. Phys. , 2013, 8(6): 771
doi: 10.1007/s11467-013-0329-5
10 X.-J. Bi, P.-F. Yin, and Q. Yuan, Front. Phys . 2013, 8(6): 794
doi: 10.1007/s11467-013-0330-z
11 M. Li, X.-D. Li, S. Wang, and Y. Wang, Front. Phys. , 2013, 8(6): 828, arXiv: 1209.0922
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