VI light curves of SMC type II Cepheids (Soszynski+, 2010)

Details VI light curves of SMC type II Cepheids (Soszynski+, 2010) VI light curves of SMC type II Cepheids (Soszynski+, 2010)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat.120600091s&link_type=abstract

VizieR On-line Data Catalog: J/AcA/60/91. Originally published in: 2010AcA....60...91S

Physics

Magellanic Clouds, Stars: Variable, Magnitudes

Scientific paper

The eighth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) contains type II Cepheids in the Small Magellanic Cloud (SMC). The sample consists of 43 objects, including 17 BL Her, 17 W Vir and 9 RV Tau stars (first examples ever found in the SMC). Seven stars have been classified as peculiar W Vir stars - a recently identified subclass of type II Cepheids. These stars have distinctive light curves, are brighter and bluer than the ordinary W Vir variables. We confirm that a large fraction of the peculiar W Vir stars are members of binary systems.
(3 data files).

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