Physical models for the UV continua of symbiotic stars

Details Physical models for the UV continua of symbiotic stars Physical models for the UV continua of symbiotic stars

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..409k&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 409-411 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Binary Stars, Interstellar Extinction, Iue, Photometry, Symbiotic Stars, Ultraviolet Spectra, Continuum Modeling, High Temperature, Line Spectra

Scientific paper

Low resolution IUE spectra represent a unique opportunity to examine the hot component in a symbiotic binary. Reddening-free color indices were developed which serve to identify the nature of the hot components in these interesting systems. The hot components are divided into two categories: (1) accreting main sequence stars; and (2) hot stellar sources. Symbiotic stars are therefore not a homogeneous group of variables, and at least two formation mechanisms are needed to produce the observed sample.

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