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2000A&A...358..462V - Astronomy and Astrophysics, volume 358462-470 (2000/6-2)
Hard X-rays emitted by starbursts as predicted by population synthesis models including a realistic fraction of interacting binaries.
VAN BEVER J. and VANBEVEREN D.
Abstract (from CDS):
We combine our close binary population number synthesis code with the formation mechanism of X-radiation in young supernova remnants and in high mass X-ray binaries, to predict the hard X-ray luminosity emitted by starbursts. We demonstrate that the impact of interacting binaries is substantial. Therefore, observations of hard X-rays with energies larger than 2 keV of starburst regions may highlight the importance of close binary evolution in understanding properties of active starformation regions.
Abstract Copyright: ∼
Journal keyword(s): stars: binaries: close - ISM: supernova remnants - galaxies: starburst - galaxies: stellar content - X-rays: stars
Simbad objects: 8
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