Please use this identifier to cite or link to this item:
Title: High mass microquasars and low latitude gamma-ray sources
Author: Bosch i Ramon, Valentí
Romero, Gustavo E.
Paredes i Poy, Josep Maria
Keywords: Estels binaris de raigs X
Raigs gamma
X-ray binaries
Gamma rays
Issue Date: 2005
Publisher: Springer Verlag
Abstract: Population studies of unidentified EGRET sources suggest that there exist at least three different populations of galactic gamma-ray sources. One of these populations is formed by young objects distributed along the galactic plane with a strong concentration toward the inner spiral arms of the Galaxy. Variability, spectral and correlation analysis indicate that this population is not homogeneous. In particular, there is a subgroup of sources that display clear variability in their gamma-ray fluxes on timescales from days to months. Following the proposal by Kaufman Bernad\'o et al. (2002), we suggest that this group of sources might be high-mass microquasars, i.e. accreting black holes or neutron stars with relativistic jets and early-type stellar companions. We present detailed inhomogeneous models for the gamma-ray emission of these systems that include both external and synchrotron self-Compton interactions. We have included effects of interactions between the jet and all external photon fields to which it is exposed: companion star, accretion disk, and hot corona. We make broadband calculations to predict the spectral energy distribution of these objects from radio up to GeV energies. The results and predictions can be tested by present and future gamma-ray instruments like INTEGRAL, AGILE, and GLAST.
Note: Versió postprint del document publicat a:
It is part of: Astronomy and Astrophysics, 2005, vol. 429, num. 1, p. 267-276
Related resource:
ISSN: 0004-6361
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

Files in This Item:
File Description SizeFormat 
517649.pdf244.92 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.