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2001MNRAS.321..421O - Mon. Not. R. Astron. Soc., 321, 421-432 (2001/March-1)
The Clusters AgeS Experiment (CASE): RR Lyrae variables in the globular cluster NGC 6362.
OLECH A., KALUZNY J., THOMPSON I.B., PYCH W., KRZEMINSKI W. and SCHWARZENBERG-CZERNY A.
Abstract (from CDS):
The V-band light curves of three of the RRc stars exhibit changes in amplitude of over 0.1mag on the time-scale of around one week. Near the radial first overtone frequency we find one or two peaks, which strongly suggests that these variables belong to the newly identified group of non-radial pulsating RR Lyr stars.
Abstract Copyright: Blackwell Science Ltd
Journal keyword(s): techniques: photometric - binaries: eclipsing - stars: fundamental parameters - stars: variables: other - globular clusters: individual: NGC 6362
Simbad objects: 48
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