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Luminosity and Mass Functions for the Pleiades from the Schmidt Survey

Published online by Cambridge University Press:  07 August 2017

E. Schilbach
Affiliation:
WIP Astronomie, Universität Potsdam, Germany
H. Meusinger
Affiliation:
Thüringer Landessternwarte Tautenburg, Germany
J. Souchay
Affiliation:
Observatoire de Paris, France

Extract

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From MAMA measurements of Tautenburg and OCA Schmidt plates we obtained proper motions and photographic UBVR photometry for ca. 45 000 stars up to B = 19 mag within a 17 square degree region in the Pleiades. An accuracy of 0.6 mag and 2 mas/year was estimated for magnitudes and proper motions, respectively. A sample of 554 cluster members was separated by use of both astrometric and photometric information on stars.

Type
Poster Papers
Copyright
Copyright © Kluwer 1995