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

  • The 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.

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Metadaten
Author:S. Meibom, S. A. Barnes, K. Covey, R. D. Jeffries, S. Matt, J. Morin, A. Palacios, A. Reiners, A. Sicilia-Aguilar, J. Irwin
DOI:https://doi.org/10.1002/asna.201211777
ISSN:0004-6337 (print)
ISSN:1521-3994 (online)
Parent Title (English):Astronomische Nachrichten = Astronomical notes
Publisher:Wiley-VCH
Place of publication:Weinheim
Document Type:Article
Language:English
Year of first Publication:2013
Year of Completion:2013
Release Date:2017/03/26
Tag:circumstellar matter; stars: late-type; stars: magnetic fields; stars: pre-main sequence; stars: rotation
Volume:334
Issue:1-2
Pagenumber:4
First Page:168
Last Page:171
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer Review:Referiert