The photometric variability of solar-type stars. I - Preliminary results for the Pleiades, Hyades, and the Malmquist Field

Details The photometric variability of solar-type stars. I - Preliminary results for the Pleiades, Hyades, and the Malmquist Field The photometric variability of solar-type stars. I - Preliminary results for the Pleiades, Hyades, and the Malmquist Field

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..934r&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Dec. 1982, p. 934-944.

Astronomy and Astrophysics

Astronomy

28

Main Sequence Stars, Pleiades Cluster, Stellar Spectra, Stellar Spectrophotometry, Variable Stars, Data Reduction, Data Systems, Star Clusters, Stellar Luminosity, Tables (Data)

Scientific paper

The young main sequence stars in the Pleiades and Hyades clusters, and old disk stars in the Malmquist Field near the north galactic pole, have been observed by precision photometry in order to determine the prevalance of variability among solar type stars. Significant variations have been found in at least five, and possibly ten, of 44 Hyades stars, and possibly one of the 41 stars in the Malmquist Field, all of which are of spectral type F8 V-K2 V.

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