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

Abstract:

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 an age of ~13 Myr. The observations were done in the I-band using 4 different telescopes and the variability study is sensitive to periods from less than 0.2 day to 20 days. Rotation periods are der...

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Publication status:
Published

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Publisher copy:
10.1051/0004-6361/201321508

Authors


Artemenko, S More by this author
Bouvier, J More by this author
Ibrahimov, M More by this author
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Journal:
ASTRONOMY and ASTROPHYSICS
Volume:
560
Pages:
A13-A13
Publication date:
2013-06-26
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:50b3fe1e-2b5f-4e50-8534-520d32303a0f
Source identifiers:
443497
Local pid:
pubs:443497
Language:
English
Keywords:

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