2004/06/22 by R. Ansari, M. Aurière, P. Baillon +20 · 3 citations
Physics and Astronomy · Engineering · #Astrophysical Phenomena and Observations #Stellar, planetary, and galactic studies #Astronomical Observations and Instrumentation
paper · pdf · doi:10.1051/0004-6361:20035659
We present the AGAPE astrometric and photometric catalogue of 1579 variable stars in a field centred on M 31. This work is the first survey devoted to variable stars in the bulge of M 31. The R magnitudes of the objects and the colours suggest that our sample is dominated by red long-period variable stars (LPV), with a possible overlap with Cepheid-like type II stars. Fits of the light curves with sinusoids suggest that a large fraction of the stars correspond to periodic or semi-periodic objects with periods longer than 100 days. Twelve nova candidates are identified. Correlations with other catalogues suggest that 2 novae could be recurrent novae and provide possible optical counterparts for 2 supersoft X-ray sources candidates observed with Chandra.