Velocities of F-G-K stars in Blanco 1 (Mermilliod+, 2008)

Details Velocities of F-G-K stars in Blanco 1 (Mermilliod+, 2008) Velocities of F-G-K stars in Blanco 1 (Mermilliod+, 2008)

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34850095m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/485/95. Originally published in: 2008A&A...485...95M

Astronomy and Astrophysics

Astrophysics

Clusters: Open, Stars: Dwarfs, Photometry: Ubvri, Proper Motions, Radial Velocities

Scientific paper

The nearby open cluster Blanco 1 is of considerable astrophysical interest for formation and evolution studies of open clusters because it is the third highest Galactic latitude cluster known. It has been observed often, but so far no definitive and comprehensive membership determination is readily available.
An observing programme was carried out to study the stellar population of Blanco 1, and especially the membership and binary frequency of the F5-K0 dwarfs.
We obtained radial-velocities with the CORAVEL spectrograph in the field of Blanco 1 for a sample of 148 F-G-K candidate stars in the magnitude range 10

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