Multiwavelength Modelling the SED of Symbiotic X-Ray Binaries

Details Multiwavelength Modelling the SED of Symbiotic X-Ray Binaries Multiwavelength Modelling the SED of Symbiotic X-Ray Binaries

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..447..233s&link_type=abstract

Evolution of compact binaries. Proceedings of a workshop held at Hotel San Martín, Viña del Mar, Chile 6–11 May 2011. ASP Confe

Astronomy and Astrophysics

Astronomy

Scientific paper

Radiation of the symbiotic X-ray binaries (SyXBs) dominates both the supersoft X-ray and the far-UV domain. Therefore, to determine their fundamental parameters, a multiwavelength approach in modelling their spectra is essential. In this contribution I introduce the composite spectrum of SyXBs and its individual components of radiation in the X-ray - near-IR continuum. Using the method of disentangling the composite spectra, fundamental parameters of individual radiative components can be determined. Here, I illustrate the multiwavelength modelling the SED for a SyXB LIN 358, and the anomalous supersoft source LIN 333 in the Small Magellanic Cloud.

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