VI light curves of LMC RR Lyrae stars (Soszynski+, 2009)

Details VI light curves of LMC RR Lyrae stars (Soszynski+, 2009) VI light curves of LMC RR Lyrae stars (Soszynski+, 2009)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat.120590001s&link_type=abstract

VizieR On-line Data Catalog: J/AcA/59/1. Originally published in: 2009AcA....59....1S

Physics

Magellanic Clouds, Stars: Variable, Magnitudes

Scientific paper

We detected one new RR Lyr star with additional eclipsing variations. The spatial distribution of RR Lyr stars in the LMC is distinctly non-spherical and it is elongated in the same direction as the LMC bar. The basic statistical features of RR Lyr stars in the LMC are provided. The apparent V-band magnitudes for RRab stars have the modal value at 19.36mag, and for overtone RR Lyr stars it is about 19.32mag. The mean periods for RRab, RRc and RRe stars are 0.576, 0.337 and 0.270-days, respectively.
(2 data files).

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