Variability of Young Solar-Type Stars in the Pleiades Open Cluster

Details Variability of Young Solar-Type Stars in the Pleiades Open Cluster Variability of Young Solar-Type Stars in the Pleiades Open Cluster

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.2301g&link_type=abstract

American Astronomical Society Meeting 210, #23.01; Bulletin of the American Astronomical Society, Vol. 39, p.128

Biology

Scientific paper

We present a preliminary report on a program of photometric monitoring of the solar-type stars in the young Pleiades open cluster. Specifically, we report on the results for 37 nights of observation in our survey region that includes 12 solar-type Pleiades members. The goal of the program is to characterize the short- and long-term brightness variability of young solar-type stars during the epoch of the formation and early evolution of young planetary atmospheres.
This work is supported in part by a joint grant from the NASA Astrobiology Institute to the University of Arizona and the NOAO/NSO. The NSO is operated by AURA under a cooperative agreement with the NSF.

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