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Stella rotation in young clusters: the first 4 million years

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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


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