The Be star HD 58050 as a new 3-hour period large amplitude β CMa variable.

Details The Be star HD 58050 as a new 3-hour period large amplitude β CMa variable. The Be star HD 58050 as a new 3-hour period large amplitude β CMa variable.

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981geoca...1.....f&link_type=abstract

GEOS Circular on Small-Amplitude Variables, No. SA 1, 7 p. (1981)

Astronomy and Astrophysics

Astrophysics

Be Stars:Beta Cma Stars, Beta Cma Stars:Light Curves, Beta Cma Stars:Periods, Beta Cma Stars:Be Stars, Light Curves, Periods

Scientific paper

HD 58050, spectral class B2V, is a Be star which has been well studied spectroscopically and shows strong emission lines of variable intensity. Although it was proved to be a photographic variable as early as 1934, it has up to now been underobserved photometrically. HD 58050 appears to this day as a unique object. It is the Be star with the shortest stable period known. Its period is 10 times shorter than that of 28 CMa, whose exceptional character had previously been pointed out. The astrophysical study of the pulsating Be star HD 58050 would open new vistas on the interpretation of the Be phenomenon.

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