Publication:
Angular momentum evolution of cool stars: Toward a synthesis of observations and theory before and after the ZAMS

Simple item page
dc.bibliographiccitation.firstpage168
dc.bibliographiccitation.issue1-2
dc.bibliographiccitation.journalAstronomische Nachrichten
dc.bibliographiccitation.lastpage171
dc.bibliographiccitation.volume334
dc.contributor.authorMeibom, S.
dc.contributor.authorBarnes, S. A.
dc.contributor.authorCovey, K. R.
dc.contributor.authorJeffries, R. D.
dc.contributor.authorMatt, S.
dc.contributor.authorMorin, Julien
dc.contributor.authorPalacios, A.
dc.contributor.authorReiners, Ansgar
dc.contributor.authorSicilia-Aguilar, A.
dc.contributor.authorIrwin, Jonathan
dc.date.accessioned2018-11-07T09:28:18Z
dc.date.available2018-11-07T09:28:18Z
dc.date.issued2013
dc.description.abstractThe coexistence of fast and slowly rotating cool stars in ZAMS clusters - forming distinct sequences in the color vs. rotation period plane - is providing clues to differences in their pre main-sequence angular momentum evolution. This Cool Stars 17 splinter was dedicated to a discussion of new observational and theoretical results that may help discriminate between proposed mechanisms for early angular momentum regulation and help us explain the observed ZAMS dichotomy. (C) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
dc.identifier.doi10.1002/asna.201211777
dc.identifier.isi000325859900039
dc.identifier.urihttps://resolver.sub.uni-goettingen.de/purl?gro-2/30738
dc.notes.statuszu prüfen
dc.notes.submitterNajko
dc.publisherWiley-v C H Verlag Gmbh
dc.relation.issn1521-3994
dc.relation.issn0004-6337
dc.titleAngular momentum evolution of cool stars: Toward a synthesis of observations and theory before and after the ZAMS
dc.typejournal_article
dc.type.internalPublicationyes
dc.type.peerReviewedyes
dc.type.statuspublished
dspace.entity.typePublication

Files

Collections

Publications