Radial velocities of {alpha} Per stars (Mermilliod+, 2008)

Details Radial velocities of {alpha} Per stars (Mermilliod+, 2008) Radial velocities of {alpha} Per stars (Mermilliod+, 2008)

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34880409m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/488/409. Originally published in: 2008A&A...488..409M

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Clusters: Open, Radial Velocities

Scientific paper

The Alpha Persei open cluster (Melotte 20) is one of the nearby clusters (d<500pc) for which a long-term systematic radial-velocity monitoring of the solar-type stars has not been published so far.
We undertook an observing program in 1982 to study the membership, duplicity, and rotation of the main-sequence stars and to compare the results with those of the other nearby clusters.
Radial-velocity observations of 60 solar-type stars in Mel 20 were obtained with CORAVEL, and of 44 fainter stars with ELODIE spectrographs, in the magnitude range 9.5

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