Photometric UBV period study of eight AP stars

Details Photometric UBV period study of eight AP stars Photometric UBV period study of eight AP stars

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pasp...93..344b&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 93, June-July 1981, p. 344-350. Research supported by the Research Corp

Astronomy and Astrophysics

Astronomy

17

A Stars, Magnetic Stars, Periodic Variations, Stellar Spectrophotometry, Variable Stars, Hertzsprung-Russell Diagram, Reference Stars, Stellar Magnitude, Ubv Spectra

Scientific paper

Eight Ap stars for which periods had been determined by Winzer (1974) were the subject of an independent period determination. All were stars which were found to be short-period variables and which showed the typical small-amplitude variation associated with short periods. For six of these, the period was confirmed. For one, HR 9017, a different and better period was determined and for the remaining star, HR 4430, periodic variation was not observed.

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