IUE spectra of the massive close binary V382 Cygni

Details IUE spectra of the massive close binary V382 Cygni IUE spectra of the massive close binary V382 Cygni

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..474k&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Aug.-Sept. 1979, p. 474-478.

Astronomy and Astrophysics

Astronomy

7

Cygnus Constellation, Eclipsing Binary Stars, Iue, Stellar Spectra, Ultraviolet Astronomy, Absorption Spectra, Emission Spectra, Interstellar Chemistry, Photosphere, Stellar Mass Ejection

Scientific paper

The massive close binary, V382 Cyg, was observed with the low-dispersion spectrograph on the IUE satellite. The dereddened spectrum can be reasonably represented by a 40,000-K model atmosphere. The spectra show interstellar, photospheric, and shell absorption blends and one shell emission feature. From one of the shell absorptions, it is possible to calculate a limiting systemic mass loss rate of about 0.00004 solar mass/yr.

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