Study of the variable stars V54, V102, and V103 in the central region of the globular cluster M5

Details Study of the variable stars V54, V102, and V103 in the central region of the globular cluster M5 Study of the variable stars V54, V102, and V103 in the central region of the globular cluster M5

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..246k&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 246; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 7, July 1992, p. 614

Astronomy and Astrophysics

Astronomy

4

Globular Clusters, Periodic Variations, Stellar Luminosity, Variable Stars, Light Curve, Stellar Spectrophotometry

Scientific paper

The periods and amplitudes of variability are determined for the
variable stars V54, V102, and V103 of Sawyer Hogg's (1973) catalog from
their photographic B-magnitudes. Both the light curves and periods of
these stars are typical of RR Lyrae variables.

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