Nr. Walborn et Js. Nichols, A LARGE, PERIODIC VARIATION IN THE STELLAR WIND OF THETA(1)-ORIONIS-C, The Astrophysical journal, 425(1), 1994, pp. 120000029-120000032
A period of 15.4 days, recently discovered by Stahl et al. from intens
ive monitoring of Halpha emission in theta1 Ori C during 1992-1993, ha
s been found to phase large variations in the C IV lambdalambda1548, 1
551 wind profile of this star previously reported from IUE high-resolu
tion data obtained during 1978-1983. These stellar-wind variations are
among the largest observed in O stars not known to be components of i
nteracting binaries; the strict periodicity is unique among apparently
single O stars and constitutes an important constraint on the unknown
origin of the phenomenon.