Variable stars in the old galactic cluster M67

Details Variable stars in the old galactic cluster M67 Variable stars in the old galactic cluster M67

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988basi...16..139r&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 16, Dec. 1988, p. 139-144.

Astronomy and Astrophysics

Astronomy

5

Astronomical Photometry, Galactic Clusters, Open Clusters, Variable Stars, Photographic Plates, Schmidt Telescopes, Stellar Magnitude

Scientific paper

Schmidt plates of the old open galactic cluster M67 were obtained on
twelve nights to find the most probable variables in the cluster. The
Sabattier technique was used to derive the magnitudes of the cluster
members. The most probable variable stars in this cluster determined by
this method are listed.

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