B and V photometry of HR 8752

Details B and V photometry of HR 8752 B and V photometry of HR 8752

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..403w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 203, Apr. 1983, p. 403-408.

Astronomy and Astrophysics

Astronomy

10

Companion Stars, Stellar Spectrophotometry, Supergiant Stars, Ubv Spectra, Variable Stars, Visual Photometry, Iue, Satellite Observation, Spaceborne Astronomy, Stellar Magnitude, Stellar Spectra

Scientific paper

B and V photoelectric magnitudes have been obtained during the years 1976 to 1978 of the spectrum-variable supergiant HR 8752, which was found to vary by more than 0.2 mag in brightness and by ≡0.1 in B-V. Significant brightness changes occur on time-scales of tens of days and possibly on shorter time-scales still. No clear relationship between photometric changes and spectral changes is discernible.

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