2008, Vol. 25(11): 4185-4188    DOI:
Non-Thermal Photon Emission from Shell-Type Supernova Remnants
DOU Ya-Nan, ZHANG Li
Department of Physics, Yunnan University, Kunming 650091
收稿日期 2008-04-16  修回日期 1900-01-01
Supporting info

[1] Reynolds S P 1996 Astrophys. J. 459 L13

[2] Slane P et al 2001 Astrophys. J. 548 814

[3] Aharonian F A et al 2005 Astron. Astrophys.
437 L7

[4] Aharonian F A et al 2006 Astrophys. J. 636
777

[5] Aharonian F A et al 2007 Astrophys. J. 661
236

[6] Katz B et al 2008 J. Cosmol. Astropart. Phys.
1 18

[7] Sturner S J et al 1997 Astrophys. J. 490 619

[8] Yamazaki R et al 2006 MNRAS 3711975

[9] Zhang L and Fang J 2007 Astrophys. J. 666 247

[10] Moraitis K et al 2007 Astron. Astrophys. 462
173

[11] Drury L O et al 1999 Astron. Astrophys. 347
370

[12] Gaisser T K et al 1998 Astrophys. J. 492
219

[13] Blondin J M et al 1998 Astrophys. J. 500 342

[14] Lazendic J S et al 2004 Astrophys. J. 602
701

[15] Bamba A et al 2005 Astrophys. J. 632295

[16] Duncan A R et al 2000 Astron. Astrophys. 364
732

[17] Enomoto R et al 2006 Astrophys. J. 652 1268

[18] Kassim N E and Weiler K W 1990 Nature 343 146

[19] Cui W and Konopelko A 2006 Astrophys. J. 652
L109