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Multiwavelength Modeling the SED of Strongly Interacting Binaries

Published online by Cambridge University Press:  23 April 2012

Augustin Skopal
Augustin Skopal*
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia email: skopal@ta3.sk
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Abstract

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The spectrum of strongly interacting binaries, as for example, high and low mass X-ray binaries, symbiotic (X-ray) binaries and/or classical and recurrent novae, consists of more components of radiation contributing from hard X-rays to radio wavelengths. To understand the basic physical processes responsible for the observed spectrum we have to disentangle the composite spectrum into its individual components, i.e. to determine their physical parameters. In this short contribution I demonstrate the method of modeling the multiwavelength SED on the example of the extragalactic super-soft X-ray source RX J0059.1-7505 (LIN 358).

Keywords

stars: fundamental parametersX-rays: individual (RX J0059.1-7505)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 65 - 66
Copyright
Copyright © International Astronomical Union 2012

References

Kahabka, P. & Haberl, F. 2006, A&A, 452, 431Google Scholar
Mürset, U., Schild, H., & Vogel, M. 1996, A&A, 307, 516Google Scholar
Skopal, A., Sekeráš, M., Gonzĺez-Riestra, R., & Viotti, R. F. 2009, A&A, 507, 1531Google Scholar