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Hard X-ray-to-radio energy distributions in starburst galaxies

Published online by Cambridge University Press:  25 May 2016

Miguel Cerviño
Affiliation:
LAEFF-INTA, P.O. Box 50727, E-28080 Madrid, Spain.
J. Miguel Mas-Hesse
Affiliation:
LAEFF-INTA, P.O. Box 50727, E-28080 Madrid, Spain.

Abstract

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We present in this contribution the predictions on the multiwavelength spectral energy distribution of our evolutionary population synthesis models including single and binary stellar systems. The high energy computations include the emission associated to X-ray binaries and supernovae remnants, as well as the mechanical energy released into the interstellar medium, which can be partially reprocessed into thermal X-rays. With these components we compute the spectral energy distribution of starburst galaxies from X-ray to radio ranges, and analyze finally the effects of the high energy emission on the H and He ionizing continuum.

Type
Part 5. Wolf-Rayet stars and other massive stars in starburst galaxies: the case of Wolf-Rayet galaxies (integrated spectra)
Copyright
Copyright © Astronomical Society of the Pacific 1999 
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