TY  - JOUR
A1  - Meibom, S.
A1  - Barnes, Sydney A.
A1  - Covey, K.
A1  - Jeffries, R. D.
A1  - Matt, S.
A1  - Morin, J.
A1  - Palacios, A.
A1  - Reiners, A.
A1  - Sicilia-Aguilar, A.
A1  - Irwin, J.
T1  - Angular momentum evolution of cool stars: Toward a synthesis of observations and theory before and after the ZAMS
JF  - Astronomische Nachrichten = Astronomical notes
N2  - 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.
KW  - circumstellar matter
KW  - stars: late-type
KW  - stars: magnetic fields
KW  - stars: pre-main sequence
KW  - stars: rotation
Y1  - 2013
U6  - https://doi.org/10.1002/asna.201211777
SN  - 0004-6337
SN  - 1521-3994
VL  - 334
IS  - 1-2
SP  - 168
EP  - 171
PB  - Wiley-VCH
CY  - Weinheim
ER  -