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IUE spectra of the massive close binary V382 Cygni (1979)

Koch, R. H. ; Fanelli, M. N. ; Siah, M. J.

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Publication Date: 2019-06-27

Description: 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.

Keywords: ASTROPHYSICS

Type: Astronomical Society of the Pacific; vol. 91

Format: text

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