Photometric variability of solar-type members of the Pleiades open cluster

Details Photometric variability of solar-type members of the Pleiades open cluster Photometric variability of solar-type members of the Pleiades open cluster

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..648g&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Physics

Photometric, Polarimetric, And Spectroscopic Instrumentation, Chromosphere, Extrasolar Planetary Systems

Scientific paper

We present some preliminary results from a program utilizing a small-aperture transit telescope for the photometric monitoring of a set of solar-type stars in the young Pleiades cluster at an age of approximately 100 Myr. The photometry sample includes 12 stars in the (B-V)0 color range of 0.58-0.76, corresponding to a range in spectral type of approximately F9 V-G9 V.

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