Physics
Scientific paper
Feb 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998kfnt...14...48k&link_type=abstract
Kinematika Fiz. Nebesn. Tel, Tom 14, No. 1, p. 48 - 51
Physics
Be Stars: Stellar Envelopes, Be Stars: H Alpha
Scientific paper
The authors analyse Hα emission line profiles in the spectrum of the Be star β CMi observed in 1987 - 1988. The following parameters are determined: equivalent width, maximum intensity, relative intensities of blue and red emission peaks (V/R), radial velocities. Rapid variations of Hα emission line profiles are found. Radial velocities of the gaseous envelope expansion are estimated.
Krugov V. D.
Vojta S. V.
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