Structure and age of the local association /Pleiades group/

Details Structure and age of the local association /Pleiades group/ Structure and age of the local association /Pleiades group/

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87...37e&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Feb. 1975, p. 37-63.

Astronomy and Astrophysics

Astronomy

95

Early Stars, Galactic Structure, Pleiades Cluster, Star Clusters, Stellar Luminosity, Stellar Motions, Astronomical Photometry, Brightness Temperature, Main Sequence Stars, Milky Way Galaxy, Red Shift, Star Distribution, Stellar Evolution, Stellar Spectrophotometry, Tables (Data)

Scientific paper

Intermediate-band indices are used to derive luminosities for some 500 early-type stars with well-determined proper motions and radial velocities. Space motion vectors and galactic coordinates are computed for the stars considered. It is found that the local association members are mainly concentrated in the Sco-Cen region in the Southern Hemisphere and the Cas-Tau region in the north.

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