@article{MeibomBarnesCoveyetal.2013,
  author    = {Meibom, S. and Barnes, Sydney A. and Covey, K. and Jeffries, R. D. and Matt, S. and Morin, J. and Palacios, A. and Reiners, A. and Sicilia-Aguilar, A. and Irwin, J.},
  title     = {Angular momentum evolution of cool stars: Toward a synthesis of observations and theory before and after the ZAMS},
  series = {Astronomische Nachrichten = Astronomical notes},
  volume    = {334},
  journal   = {Astronomische Nachrichten = Astronomical notes},
  number    = {1-2},
  publisher = {Wiley-VCH},
  address   = {Weinheim},
  issn      = {0004-6337},
  doi       = {10.1002/asna.201211777},
  pages     = {168 -- 171},
  year      = {2013},
  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.},
  language  = {en}
}