- Abstract:
-
We report on the results of a time-series photometric survey of NGC 2362, carried out using the CTIO 4-m Blanco telescope and Mosaic-II detector as part of the Monitor project. Rotation periods were derived for 271 candidate cluster members over the mass range 0.1 ≲ M/M⊙ ≲ 1.2. The rotation period distributions show a clear mass-dependent morphology, qualitatively similar to that in NGC 2264, as would be expected from the age of this cluster. Using models of angular momentum evolution, we sho...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2007.12725.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 384
- Issue:
- 2
- Pages:
- 675-686
- Publication date:
- 2008-02-21
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:b180634d-1ec8-493b-823d-456dc1784f22
- Source identifiers:
-
158098
- Local pid:
- pubs:158098
- Language:
- English
- Keywords:
- Copyright date:
- 2008
Journal article
The Monitor project: rotation of low-mass stars in NGC 2362 - testing the disc regulation paradigm at 5 Myr
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