UV and optical spectroscopy of W Serpentis objects

Details UV and optical spectroscopy of W Serpentis objects UV and optical spectroscopy of W Serpentis objects

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..411s&link_type=abstract

In ESA 4th European IUE Conf. p 411-413 (SEE N84-35135 24-88)

Computer Science

Binary Stars, Optical Emission Spectroscopy, Stellar Evolution, Ultraviolet Spectroscopy, Continuous Radiation, Iue, Stellar Composition, Stellar Envelopes

Scientific paper

Ultraviolet (IUE) and optical spectroscopic observations of W Serpentis objects (W Ser, W Cru, AR Pav, RX Cas, SX Cas) were analyzed. Results indicate the presence of circumstellar plasma with high degree of ionization. These objects are believed to be near contact or even contact systems, presently in an evolutionary stage, where a common envelope is formed.

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