Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...358..462v&link_type=abstract
Astronomy and Astrophysics, v.358, p.462-470 (2000)
Astronomy and Astrophysics
Astrophysics
43
Stars: Binaries: Close, Ism: Supernova Remnants, Galaxies: Starburst, Galaxies: Stellar Content, X-Rays: Stars
Scientific paper
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.
van Bever J.
Vanbeveren Dany
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