RR Lyrae variables in M5 as a test of pulsational theory

被引:27
作者
Caputo, F
Castellani, V
Marconi, M
Ripepi, V
机构
[1] Osserv Astron Capodimonte, I-80131 Naples, Italy
[2] Univ Pisa, Dipartimento Fis, I-56100 Pisa, Italy
关键词
stars : horizontal branch; stars : variables : other; globular clusters : general; globular clusters : individual : M5; distance scale;
D O I
10.1046/j.1365-8711.1999.02561.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present B and V CCD photometry for variables in the cluster central region, adding new data for 32 variables and giving suitable light curves, mean magnitudes and corrected colours for 17 RR Lyrae variables. Adding the data given in this paper to similar data that have already appeared in the literature, we discuss a sample of 42 variables, as given by 22 RRab and 20 RRc, in the light of recent predictions from pulsational theories. We find that the observational evidence concerning M5 pulsators appears in marginal disagreement with predictions concerning the colour of the first overtone blue edge (FOBE), whereas a clear disagreement appears between the zero-age horizontal branch (ZAHB) luminosities predicted through evolutionary and pulsational theories.
引用
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页码:815 / 827
页数:13
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