Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS

Details Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS Long Period Variables in the Magellanic Clouds: OGLE + 2MASS + DENIS

2004-04-28

arxiv.org/abs/astro-ph/0404561v1

Astron.Astrophys. 425 (2004) 595-613

Astronomy and Astrophysics

Astrophysics

Astronomy and Astrophysics, accepted

Scientific paper

10.1051/0004-6361:20047098

(abridged) The 68000 I-band light curves of variable stars detected by the OGLE survey in the Large and Small Magellanic Clouds (MCs) are fitted by Fourier series, and also correlated with the DENIS and 2MASS databases and with lists of spectroscopically confirmed M-, S- and C-stars. Lightcurves and the results of the lightcurve fitting (periods and amplitudes) and DENIS and 2MASS magnitudes are presented for 2277 M-,S-,C-stars in the MCs. The following aspects are discussed: the K-band period-luminosity relations for the spectroscopically confirmed AGB stars, period changes over a timespan of about 17 years in a subset of about 400 LPVs, and candidate obscured AGB stars.

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