Reconstruction of the SED in the UV/optical/IR continuum of symbiotic binaries

Details Reconstruction of the SED in the UV/optical/IR continuum of symbiotic binaries Reconstruction of the SED in the UV/optical/IR continuum of symbiotic binaries

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..367s&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

Scientific paper

We reconstruct the composite spectral energy distribution (SED) in the continuum between 0.12 and 5 μ of symbiotic binaries by a three-component model of radiation. Two stellar components are from the hot and the cool star, while the nebular radiation is from the ionized circumbinary medium. We demonstrate this method on examples of symbiotic stars in quiescent phase (EG And) and in outburst (CI Cyg).

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