The high-latitude blue variable PHL 346 and helium-weak star PHL 382

Details The high-latitude blue variable PHL 346 and helium-weak star PHL 382 The high-latitude blue variable PHL 346 and helium-weak star PHL 382

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..727k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, June 15, 1990, p. 727-730.

Astronomy and Astrophysics

Astronomy

16

B Stars, Blue Stars, Cepheid Variables, Stellar Luminosity, Astronomical Photometry, Periodic Variations

Scientific paper

Photoelectric BV photometry of the high-latitude blue star PHL 346 in
1988 confirms earlier findings that the star is variable with a period
of 0.15231 d, that it is probably singly periodic and of Beta Cephei
type. The high-latitude blue star PHL 382 is found to be very
helium-weak, and is also suspected of photometric variability.

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