Stellar Coronae at 250 Myr: Chandra Observations of NGC 3532

Details Stellar Coronae at 250 Myr: Chandra Observations of NGC 3532 Stellar Coronae at 250 Myr: Chandra Observations of NGC 3532

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642104s&link_type=abstract

American Astronomical Society, AAS Meeting #216, #421.04; Bulletin of the American Astronomical Society, Vol. 41, p.833

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Scientific paper

We present preliminary results of a Chandra observation of the 250 Myr open cluster NGC 3532, one of the best studied clusters for rotation periods between Pleiades and Hyades ages. We detect over 30 stars spanning a wide range in rotation period. We discuss the cluster's X-ray distribution function, rotation-activity relationship, and how X-ray flux and temperature vary along the cluster's rotational sequences. We compare the results with other clusters, and draw implications for the evolution of rotation and activity in young stars.

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