New results on OGLE Cepheids and PL relations in the LMC and SMC

Details New results on OGLE Cepheids and PL relations in the LMC and SMC New results on OGLE Cepheids and PL relations in the LMC and SMC

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..310...75u&link_type=abstract

Variable Stars in the Local Group, IAU Colloquium 193, Proceedings of the conference held 6-11 July, 2003 at Christchurch, New Z

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of the search for pulsating variable stars in the Magellanic Cloud fields covering the central parts of these galaxies. The data were collected during the second phase of Optical Gravitational Lensing Experiment survey (OGLE-II) from 1997 to 2000. In total, several thousand pulsating stars (Cepheids, RR Lyr) were found in both Magellanic Clouds. The photometric data of all objects are available to the astronomical community from the OGLE Internet archive. We present basic properties of pulsating stars in the Magellanic Clouds including Period-Luminosity relations for Cepheids. We also discuss observational prospects for the pulsating star field in the ongoing third phase of the OGLE project (OGLE-III) which started in 2001

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