89 Herculis and HD 161796 in 1986 and 1987

Details 89 Herculis and HD 161796 in 1986 and 1987 89 Herculis and HD 161796 in 1986 and 1987

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..171f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Feb. 1989, p. 171-174.

Astronomy and Astrophysics

Astronomy

8

Astronomical Photometry, F Stars, Ubv Spectra, Variable Stars, Hercules Nova, Light Curve, Supergiant Stars

Scientific paper

Data from UBV photometric observations of two UU Herculis stars, 89 Her
and HD 161796, are presented for the period from 1986 to 1987. Light
curves are presented for both stars in both years. The results show that
the light curve of HD 161796 is much less stable than that of 89 Her.
The periodicities and phasing of the light curves are discussed.

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