UVBY photometry of the suspected variable stars 53 Tauri, 68 Tauri, HR 4072, and HR 6096

Details UVBY photometry of the suspected variable stars 53 Tauri, 68 Tauri, HR 4072, and HR 6096 UVBY photometry of the suspected variable stars 53 Tauri, 68 Tauri, HR 4072, and HR 6096

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...269..411a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 269, no. 1-2, p. 411-414.

Astronomy and Astrophysics

Astrophysics

12

A Stars, Astronomical Photometry, Ubv Spectra, Variable Stars, B Stars, Electrophotometry

Scientific paper

Stromgren uvby photometry of four suspected variable stars is presented. Observations made at the Four College Automated Photoelectric Telescope show that the two mercury-manganese stars 53 Tauri and HR 4072 and the metallic lined star 68 Tauri are non-variable on time scales of a few days to within the accuracy of the observations. HR 6096, which has been classified as a mild silicon star, is not found to be variable and may be a metal-rich normal B star.

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