In Quest of the Secondary in the Optical Spectrum of the Interacting Binary V367-CYGNI

Details In Quest of the Secondary in the Optical Spectrum of the Interacting Binary V367-CYGNI In Quest of the Secondary in the Optical Spectrum of the Interacting Binary V367-CYGNI

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...277..480s&link_type=abstract

Astronomy and Astrophysics, Vol. 277, NO. 2/OCT(I), P. 480, 1993

Astronomy and Astrophysics

Astrophysics

2

Binaries: Close - Stars: Individual: V 367 Cyg - Accretion Disk

Scientific paper

The detection of the secondary in the optical spectrum of the
interacting binary V 367 Cyg is examined on the basis of new CCD
observations. Based on the only visible stellar line, MgII λ4481,
no indication of the secondary's component could be found. The proposed
secondary's line is due to a Fe I shell line.

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