Disentangling the composite continuum of symbiotic binaries I. S-type systems

Details Disentangling the composite continuum of symbiotic binaries I. S-type systems Disentangling the composite continuum of symbiotic binaries I. S-type systems

2005-07-12

arxiv.org/abs/astro-ph/0507272v1

Astronomy and Astrophysics

Astrophysics

37 pages in printed format, 27 figures, 4 tables, accepted for publication in Astronomy and Astrophysics

Scientific paper

10.1051/0004-6361:20034262

We describe a method of disentangling the composite,0.12-5 microns continuum of symbiotic binaries.The observed SED is determined by the IUE/HST archival spectra and flux-points corresponding to the optical UBVRI and infrared JHKLM photometric measurements. The modeled SED is given by superposition of fluxes from the cool giant, hot stellar source and nebula including the effect of the Rayleigh scattering process and considering influence of the iron curtain absorptions.We applied this method to 21 S-type symbiotic stars during quiescence, activity and eclipses.

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