Time-Dependent Synchrotron and Compton Spectra from Microquasar Jets

被引：0
|
作者：
S. Gupta
M. Böttcher
机构：
[1] Ohio University,Astrophysical Institute, Department of Physics and Astronomy
来源：
Astrophysics and Space Science | 2007年 / 307卷
关键词：
Gamma-rays: theory; Radiation mechanisms: non-thermal; X-rays: binaries;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Jet models for the high-energy emission of Galactic X-ray binary sources have regained significant interest with detailed spectral and timing studies of the X-ray emission from microquasars, the recent detection by the HESS collaboration of very-high-energy γ-rays from the microquasar LS 5039, and the earlier suggestion of jet models for ultraluminous X-ray sources observed in many nearby galaxies. Here we study the synchrotron and Compton signatures of time-dependent electron injection and acceleration, and adiabatic and radiative cooling in the jets of Galactic microquasars.
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页码：237 / 240
页数：3
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