Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..101a&link_type=abstract
(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones
Astronomy and Astrophysics
Astronomy
21
Late Stars, Stellar Spectra, Symbiotic Stars, Variable Stars, Hot Stars, Infrared Astronomy, Main Sequence Stars, Mira Variables, Stellar Evolution, Ultraviolet Astronomy, White Dwarf Stars
Scientific paper
Symbiotic stars are characterized in a review of observational investigations and theoretical models; observations outside the visible wavelengths and interacting-binary models are emphasized. X-ray, UV, optical, IR, and radio studies are summarized, and the nature of the hot star and its outbursts is discussed. Several objects are examined separately, including the probable single star V1016 Cyg, the misleading object RX Pup, the classical accretion stars CI Cyg and T CrB, the long-period Mira variable H1-36, the cool-dust object HD 330036, and symbiotic stars in the Magellanic Clouds. The significance of the unidentified 683-nm band found in about half the symbiotic stars, the status of theoretical mass-transfer models, and the kinds of observations needed to clarify the many outstanding problems are considered.
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