Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables

D. Minniti; C. Alcock; R. A. Allsman; D. R. Alves; T. S. Axelrod; A. Becker; D. P. Bennett; K. H. Cook; K. C. Freeman; K. Griest; S. L. Marshall; B. A. Peterson; M. R. Pratt; P. J. Quinn; A. W. Rodgers; C. W. Stubbs; W. Sutherland; A. Tomaney; T. Vandehei; D. L. Welch

arXiv · astro-ph/9712048

Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables

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Abstract

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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D. Minniti, C. Alcock, R. A. Allsman, D. R. Alves, T. S. Axelrod, A. Becker, D. P. Bennett, K. H. Cook, K. C. Freeman, K. Griest, S. L. Marshall, B. A. Peterson, M. R. Pratt, P. J. Quinn, A. W. Rodgers, C. W. Stubbs, W. Sutherland, A. Tomaney, T. Vandehei, D. L. Welch. 1997-12-03. Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables. https://arxiv.org/abs/astro-ph/9712048

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