Close binaries - Abundances and mass loss

Details Close binaries - Abundances and mass loss Close binaries - Abundances and mass loss

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990basi...18..261p&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 18, Sept.-Dec. 1990, p. 261-276.

Astronomy and Astrophysics

Astronomy

Abundance, Eclipsing Binary Stars, Stellar Evolution, Stellar Mass Ejection, Stellar Spectra, Metallicity, Planetary Nebulae, Stellar Atmospheres, Symbiotic Stars

Scientific paper

The abundances and mass loss aspects of close binary systems are
discussed. Emphasis is given to Algol systems, including V453 Sco, V 356
Sgr, RY Scuti, and W Serpentis. Hydrogen-poor close binary systems,
symbiotic stars, PNe with close binary central stars, and barium and
related stars are also addressed.

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