Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables
Minniti, D. · Alcock, C. · Allsman, R. A. · Alves, D. R. · Axelrod, T. S. · Becker, A. · Bennett, D. P. · Cook, K. H. · Freeman, K. C. · Griest, K. · Marshall, S. L. · Peterson, B. A. · Pratt, M. R. · Quinn, P. J. · Rodgers, A. W. · Stubbs, C. W. · Sutherland, W. · Tomaney, A. · Vandehei, T. · Welch, D. L.
Original · EN
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with special emphasis on the red semiregular stars. Based on period, amplitude and color cuts, we have selected a sample of 2000 semiregular variables with 15<P<100 days. Their color-magnitude diagram is presented, and period-luminosity relation is studied, as well as their spatial distribution. We find that they follow the bar, unlike the RR Lyrae in these fields.
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