Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197...81h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 197, Oct. 1981, p. 81-94. Research supported by the Science Research Co
Astronomy and Astrophysics
Astronomy
37
Astrometry, B Stars, Helium, Pulsars, Stellar Oscillations, Variable Stars, Line Spectra, Radial Velocity, Stellar Magnitude, Stellar Mass, Stellar Spectra, Stellar Spectrophotometry
Scientific paper
The velocity curve of the variable helium star BD + 13 deg 3224 has been determined and shown to be pulsating. By combining the velocity data with photometry, the mean radius has been deduced to be 1.6 plus or minus 0.2 solar radius, and by taking log g from neutral helium line profiles, the mass has been determined to be 0.9 +0.5, -0.3 solar mass. The gravity and composition are different from those of extreme helium stars but more similar to HD 144941.
Hill Philip W.
Kilkenny Dave
Schoenberner Detlef
Walker Helen J.
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