HD 80859 (B5 V) - A possible new slowly pulsating B-type star

Details HD 80859 (B5 V) - A possible new slowly pulsating B-type star HD 80859 (B5 V) - A possible new slowly pulsating B-type star

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...259..574v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 259, no. 2, p. 574-576.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Photometry, B Stars, Early Stars, Stellar Oscillations, Stellar Spectra, Variable Stars, Interstellar Extinction, Stellar Rotation, Ubv Spectra

Scientific paper

The VBLUW photometry of a possible new member of the slowly pulsating
B-type stars is presented and discussed. This is HD 80859 (B5 V) with a
light amplitude in the visual of 0.02m and a period P = 2.862d. Data on
the period of light variations and interstellar reddening are examined.

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