Rotation in NGC 2362: Examining the Role of Disk-Locking at 5 Myr

Details Rotation in NGC 2362: Examining the Role of Disk-Locking at 5 Myr Rotation in NGC 2362: Examining the Role of Disk-Locking at 5 Myr

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..361h&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

Star Formation, Magnetic And Electric Fields, Polarization Of Starlight, Pulsations, Oscillations, And Stellar Seismology

Scientific paper

We have obtained rotation periods for 95 stars in the young open cluster
NGC 2362 (t~5 Myr, d~1.5 kpc) and find periods ranging from P<1 day
to P~14 days. These periods have been combined with flux measurements
from archival Spitzer/IRAC images to examine the role disk-locking may
play at this age.

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