HR 3562 and 3600 - Two short-period B-type variables

Details HR 3562 and 3600 - Two short-period B-type variables HR 3562 and 3600 - Two short-period B-type variables

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..621b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 223, Dec. 1, 1986, p. 621-627.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photometry, B Stars, Variable Stars, Light Curve, Radial Velocity, Reference Stars

Scientific paper

From intensive photometric observations of the early B stars HR 3562 and HR 3600, the authors show that they are both singly periodic variables. The multiple periods previously proposed are not confirmed and an explanation in terms of non-radial oscillations need not be invoked. The authors suggest that they be classified as ellipsoidal variables rather than 53 Per stars. One of the comparison stars, HR 3527, is an eclipsing binary.

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