Short-term photometric variability of Psi Persei and Zeta Tauri

Details Short-term photometric variability of Psi Persei and Zeta Tauri Short-term photometric variability of Psi Persei and Zeta Tauri

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..131p&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 106, no. 696, p. 131-133

Astronomy and Astrophysics

Astronomy

6

B Stars, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Ultraviolet Photometry, Cassegrain Antennas, Iue, Periodic Variations

Scientific paper

We report the short-term photometric periods and UBV light and color amplitudes of the Be stars Psi Persei and Zeta Tauri, derived from observations made in Arizona and Hungary, as part of a multiwavelength campaign in 1991. The most likely periods are 1.021 and 0.665 days, respectively, with the period of Zeta Tauri being most uncertain. These are in satisfactory agreement with the periods obtained from simultaneous UV photometry and/or from previous ground-based observations.

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