The Monitor project: rotation periods of low-mass stars in M50

Jonathan Irwin , Suzanne Aigrain , Jerome Bouvier (1) , Leslie Hebb , Simon Hodgkin , Mike Irwin , Estelle Moraux (1)

1 LAOG - Laboratoire d'Astrophysique de Grenoble

We report on the results of a time-series photometric survey of M50 (NGC 2323), a ~130Myr open cluster, carried out using the Cerro Tololo Inter-American Observatory (CTIO) 4-m Blanco telescope and Mosaic-II detector as part of the Monitor project. Rotation periods were derived for 812 candidate cluster members over the mass range 0.2 <~ M/Msolar <~ 1.1. The rotation period distributions show a clear mass-dependent morphology, statistically indistinguishable from those in NGC 2516 and M35 taken from the literature. Due to the availability of data from three observing runs separated by ~10 and 1month time-scales, we are able to demonstrate clear evidence for evolution of the photometric amplitudes, and hence spot patterns, over the 10month gap. We are not able to constrain the time-scales for these effects in detail due to limitations imposed by the large gaps in our sampling, which also prevent the use of the phase information.

Domaines: Planète et Univers [physics]

Jonathan Irwin, Suzanne Aigrain, Jerome Bouvier, Leslie Hebb, Simon Hodgkin, et al.. The Monitor project: rotation periods of low-mass stars in M50. Monthly Notices of the Royal Astronomical Society, 2009, 392, pp.1456. ⟨10.1111/j.1365-2966.2008.14158.x⟩. ⟨hal-00479883⟩