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.

Topics
Open clusters
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© 2009 American Institute of Physics.
2009
American Institute of Physics
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