The Milky Way field around NGC 7635 in Cassiopeia. I - The variable stars

Details The Milky Way field around NGC 7635 in Cassiopeia. I - The variable stars The Milky Way field around NGC 7635 in Cassiopeia. I - The variable stars

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26as...24....1r&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 24, Apr. 1976, p. 1-27.

Astronomy and Astrophysics

Astronomy

11

Milky Way Galaxy, Star Distribution, Variable Stars, Infrared Astronomy, Light Curve, M Stars, Mira Variables, Star Clusters

Scientific paper

This paper gives the results of a blue and infrared study of new and old variable stars within a field of 30 sq deg centered on the nebula NGC 7635. Twenty-six variables or suspected variables are already known, and thirty-two new variable stars have been examined on plates obtained from 1962 to 1973. Types, elements, and light curves are given. Most of the new variables belong to the Mira type. They are barely visible or invisible in the blue, but fairly strong in the infrared, with B-I color indices larger than +6. Some general considerations follow.

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