89 Herculis and HD 161796 in 1988

Details 89 Herculis and HD 161796 in 1988 89 Herculis and HD 161796 in 1988

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..442f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, April 1990, p. 442-445.

Astronomy and Astrophysics

Astronomy

10

F Stars, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Electrophotometers, Light Curve, Stellar Luminosity, Stellar Mass, Telescopes

Scientific paper

New UBV photometry of V441 Herculis (89 Herculis) and 814 Herculis (HD 161796) obtained with the automatic photoelectric telescope service is presented. These two stars are members of a class of variable known as UU Herculis stars, high-latitude F supergiants that have curious properties. The intention behind the ongoing photometry is to obtain sufficient data with which to study the systematics of the variability of the stars.

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