Rotation and Magnetic Activity in the Young Open Cluster Blanco 1.

Details Rotation and Magnetic Activity in the Young Open Cluster Blanco 1. Rotation and Magnetic Activity in the Young Open Cluster Blanco 1.

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..353c&link_type=abstract

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

Other

Star Formation, X-Ray, Magnetic And Electric Fields, Polarization Of Starlight

Scientific paper

We present a study into the rotation and magnetic activity of the young (60-100 Myr), nearby (250 pc) open cluster Blanco 1, combining recently published spectroscopic and X-ray datasets. We use new V sin i and X-ray luminosity measurements, in addition to a recently completed standardized BVIc CCD survey, to probe how fundamental stellar parameters, such as X-ray emission and rotation rate, change as a function of mass in Blanco 1. Comparing our new analysis with the existing rotation-activity distributions for other open clusters, we investigate the age-dependence of angular momentum and magnetic activity among early epoch (<1 Gyr) solar-type stars, and more specifically, how Blanco 1 agrees or disagrees with the age-rotation-activity paradigm at 100 Myr.

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