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  4. Membership, binarity, and rotation of red dwarfs in the nearby open cluster Coma Berenices (Melotte 111)
 
research article

Membership, binarity, and rotation of red dwarfs in the nearby open cluster Coma Berenices (Melotte 111)

Mermilliod, J.-C.  
•
Grenon, M.
•
Mayor, M.
2008
Astronomy & Astrophysics

Context. Although several attempts have been made to identify solar-type members on the main sequence of the nearby open cluster Coma Berenices (Mel 111), the population of the lower main sequence is still poorly known.

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Type
research article
DOI
10.1051/0004-6361:200810242
Web of Science ID

WOS:000261152900035

Author(s)
Mermilliod, J.-C.  
Grenon, M.
Mayor, M.
Date Issued

2008

Published in
Astronomy & Astrophysics
Volume

491

Start page

951

End page

960

Subjects

Galaxy: open clusters and associations: individual: Coma Berenices (Melotte 111)

•

stars: binaries: spectroscopic

•

technique: radial velocities

•

North Galactic Pole

•

A-Type Stars

•

Chemical-Composition

•

Pleiades Cluster

•

Velocities

•

Praesepe

•

Photometry

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Lithium

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Region

•

Hyades

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
LASTRO  
Available on Infoscience
November 30, 2010
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/60826
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