The Monitor Project: Stellar rotation at 13~Myr: I. A photometric monitoring survey of the young open cluster h~Per

We aim at constraining the angular momentum evolution of low mass stars by measuring their rotation rates when they begin to evolve freely towards the ZAMS, i.e. after the disk accretion phase has stopped. We conducted a multi-site photometric monitoring of the young open cluster h Persei that has a...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2013-06
Hauptverfasser:	Moraux, E, Artemenko, S, Bouvier, J, Irwin, J, Ibrahimov, M, Magakian, T, Grankin, K, Nikogossian, E, Cardoso, C, Hodgkin, S, Aigrain, S, Movsessian, T A
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Angular momentum Clusters Decoupling Low mass stars Monitoring Photometry Physics - Solar and Stellar Astrophysics Space telescopes Stars Stellar evolution Stellar rotation
Online-Zugang:	Volltext
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