Photometric properties of symbiotic stars and the nature of the cool component

Details Photometric properties of symbiotic stars and the nature of the cool component Photometric properties of symbiotic stars and the nature of the cool component

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...255..171w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 255, no. 1-2, p. 171-180.

Astronomy and Astrophysics

Astronomy

51

Giant Stars, Stellar Color, Stellar Spectra, Symbiotic Stars, Astronomical Photometry, Infrared Astronomy, Interstellar Extinction

Scientific paper

The interpretation of broad-band optical and infrared colors of symbiotic stars is discussed. A comparison of the near-infrared and IRAS characteristics of S-type symbiotics and nonsymbiotic M-giants suggests that, although different from bright local M-giants, the symbiotic stars are very similar to the M-giants found in the Bulge and elsewhere. Possible interpretations of this similarity are considered.

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