On the problem of the luminous emission line stars

Details On the problem of the luminous emission line stars On the problem of the luminous emission line stars

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985msngr..39...30v&link_type=abstract

ESO Messenger (ISSN 0722-6691), March 1985, p. 30-33.

Physics

Emission Spectra, Magellanic Clouds, Stellar Envelopes, Stellar Luminosity, Stellar Spectra, Ultraviolet Spectra, Variable Stars, Cosmic Dust, H Alpha Line, Light Curve, Milky Way Galaxy, Supergiant Stars

Scientific paper

Superluminous emission-line stars in the Galaxy and Magellanic Clouds are characterized in a review of recent ESO optical and IUE UV observations. The data are presented graphically, and consideration is given to the emission lines most frequently observed, the high-resolution H-alpha profiles, the sharp variability of the S Dor variables, the smaller transient phenomena of P Cyg and Eta Car, and the role of circumstellar dust.

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