H. Schneider et al., IN QUEST OF THE SECONDARY IN THE OPTICAL-SPECTRUM OF THE INTERACTING BINARY V-367 CYGNI, Astronomy and astrophysics, 277(2), 1993, pp. 480-482
The detection of the secondary in the optical spectrum of the interact
ing binary V 367 Cyg is examined on the basis of new CCD observations.
Based on the only visible stellar line, MgII lamda4481, no indication
of the secondary's component could be found. The proposed secondary's
line is due to a Fel shell line.