Abstract
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.
Original language | English |
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Pages (from-to) | 168 |
Journal | Astronomische Nachrichten |
Volume | 334 |
Issue number | 1 |
DOIs | |
Publication status | Published - 1 Feb 2013 |
Keywords
- circumstellar matter
- stars: late-type
- stars: magnetic fields
- stars: pre-main sequence
- stars: rotation