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1994PASP..106..131P - Publ. Astron. Soc. Pac., 106, 131-133 (1994/February-0)

Short-term photometric variability of psi Persei and zeta Tauri.

PERCY J.R., IVANS I.I., FRIED R.E. and PAPARO M.

Abstract (from CDS):

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 multi-wavelength campaign in 1991. The mostlikely 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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