Stella rotation in young clusters: the first 4 million years

Rebull, L. M.; Wolfe,  S. C.; Strom,  S. E.

dc.contributor.author	Rebull, L. M.	en_US
dc.contributor.author	Wolfe, S. C.	en_US
dc.contributor.author	Strom, S. E.	en_US
dc.date.accessioned	2004-09-16T23:55:32Z
dc.date.available	2004-09-16T23:55:32Z
dc.date.issued	2004-02	en_US
dc.identifier.citation	Astronomical journal, vol. 127, pp.1029-1051	en_US
dc.identifier.citation	Pasadena, CA, USA	en_US
dc.identifier.clearanceno	03-2760	en_US
dc.identifier.uri	http://hdl.handle.net/2014/7952
dc.description.abstract	To investigate what happens to angular momentum during the earliest observable phases of stellar evolution, we searched the literature for periods (P), projected rotational velocities (v sin i), and supporting data on K5M2 stars (corresponding to masses 0.251 M) from the Orion Nebula Cluster and environs, Ophiuchi, TW Hydra, Taurus-Auriga, NGC 2264, Chamaeleon, Lupus, and Chamaeleonis.	en_US
dc.format.extent	597655 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	stars rotation	en_US
dc.title	Stella rotation in young clusters: the first 4 million years	en_US