Time-Dependent Synchrotron and Compton Spectra from Microquasar Jets

Details Time-Dependent Synchrotron and Compton Spectra from Microquasar Jets Time-Dependent Synchrotron and Compton Spectra from Microquasar Jets

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.307..237g&link_type=abstract

Astrophysics and Space Science, Volume 307, Issue 1-3, pp. 237-240

Astronomy and Astrophysics

Astrophysics

Gamma-Rays: Theory, Radiation Mechanisms: Non-Thermal, X-Rays: Binaries

Scientific paper

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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