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Cited article:
J. Bouvier
Astron. Astrophys. Suppl. Ser., 120 1 (1996) 127-138
Published online: 1996-11-15
This article has been cited by the following article(s):
7 articles
Are the spin axes of stars randomly aligned within a cluster?
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Membership and binarity of solar-type dwarfs in the nearby open cluster Alpha Persei (Mel 20)
J.-C. Mermilliod, D. Queloz and M. Mayor Astronomy & Astrophysics 488 (1) 409 (2008) https://doi.org/10.1051/0004-6361:200810016
Stellar Rotation in Young Clusters: The First 4 Million Years
L. M. Rebull, S. C. Wolff and S. E. Strom The Astronomical Journal 127 (2) 1029 (2004) https://doi.org/10.1086/380931
Why Are the K Dwarfs in the Pleiades So Blue?
John R. Stauffer, Burton F. Jones, Dana Backman, et al. The Astronomical Journal 126 (2) 833 (2003) https://doi.org/10.1086/376739
The "rotation-activity connection": Its extension to photospheric activity diagnostics
S. Messina, M. Rodonò and E. F. Guinan Astronomy & Astrophysics 366 (1) 215 (2001) https://doi.org/10.1051/0004-6361:20000201
Rotational Velocities of Low-Mass Stars in the Pleiades and Hyades
Donald M. Terndrup, John R. Stauffer, Marc H. Pinsonneault, et al. The Astronomical Journal 119 (3) 1303 (2000) https://doi.org/10.1086/301259
Rotation Periods of Late‐Type Stars in the Young Open Cluster IC 2602
Sydney A. Barnes, Sabatino Sofia, Charles F. Prosser and John R. Stauffer The Astrophysical Journal 516 (1) 263 (1999) https://doi.org/10.1086/307091