Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..151p&link_type=abstract
In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi
Physics
Angular Velocity, Optical Emission Spectroscopy, Spectrum Analysis, Stellar Rotation, X Ray Sources, B Stars, Beryllium, Inclination, Parameter Identification, Stellar Spectra
Scientific paper
Analysis of optical spectra of HD102567 (HEN 715), the optical counterpart of the X-ray source 4U1145-61, is presented. Estimates of the star's rotation velocity, inclination angle, and distance and envelope characteristics are given. Some consequences of the possible existence of a 190d orbital period for this Be/X-ray source are discussed.
Chevalier Clément
Ilovaisky Sergio A.
Pacheco Eduardo Janot
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