Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94..333m&link_type=abstract
Astronomy and Astrophysics, vol. 94, no. 2, Feb. 1981, p. 333-337. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astrophysics
10
Eclipsing Binary Stars, H Lines, Stellar Envelopes, Stellar Spectra, B Stars, Emission Spectra, H Alpha Line, H Beta Line
Scientific paper
Repeated spectroscopic observations have been made at medium dispersion of the egress phase of the VV Cep eclipsing binary system. The double emission profiles of H beta and H alpha showed characteristic variations. The blue emission component reappeared first followed by the red one. This agrees with the corresponding results obtained during the ingress phase. A rapidly rotating oblate envelope around the hot companion is proposed as a model for the emission region. The contact epochs of the different emission components allow conclusions on the morphology of the envelope.
Moellenhoff Claus
Schaifers K.
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