RESONANT COMPTON-SCATTERING AND GAMMA-RAY BURST CONTINUUM SPECTRA

被引：1

作者：

BARING, MG

机构：

[1] NASA Goddard Space Flight Center, Greenbelt, MD 20771

来源：

GAMMA RAY ASTRONOMY | 1995年 / 15卷 / 05期

关键词：

D O I：

10.1016/0273-1177(94)00042-Y

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Thomson limit of resonant inverse Compton scattering in the strong magnetic fields of neutron stars is considered as a mechanism for producing gamma-ray burst continuum spectra. Photon production spectra and electron cooling rates are presented using the full magnetic Thomson cross-section. Model emission spectra are obtained as self-consistent solutions of a set of photon and electron kinetic equations, displaying spectral breaks and other structure at gamma-ray energies.

引用

页码：85 / 88

页数：4

共 10 条

[1]

Baring M. G., 1994, AIP C P, V307, P572

[2]

BARING MG, 1995, UNPUB

[3] MULTIPLE RESONANT SCATTERING IN THE COMPTON UPSCATTER MODEL OF GAMMA-RAY BURSTS [J].