Rc light curves of 7 variables in M37 (Kiss+, 2001)

Details Rc light curves of 7 variables in M37 (Kiss+, 2001) Rc light curves of 7 variables in M37 (Kiss+, 2001)

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..33760561k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/376/561. Originally published in: 2001A&A...376..561K

Physics

Clusters: Open, Stars: Variable, Photometry: Ccd, Photometry: Cousins

Scientific paper

A CCD photometric study of the dense galactic open cluster M 37 is discussed. The majority of the analysed data have been obtained through an RC filter in order to collect time-series measurements. The observations were carried out on seven nights between December 1999 and February 2000, and have led to the discovery of 7 new variable stars in the field. Three of them have been unambiguously identified as W UMa-type eclipsing binaries, while two more are monoperiodic pulsating stars, most probably high-amplitude δ Scuti-type variables. Two stars seem to be long-period eclipsing binaries without firm period determination. The individual light curve data are presented here. (8 data files).

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