The RR Lyrae period-amplitude relation as a clue to the origin of the Oosterhoff dichotomy

被引:55
作者
Clement, CM [1 ]
Shelton, I
机构
[1] Univ Toronto, Dept Astron, Toronto, ON M5S 3H8, Canada
[2] Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA
基金
加拿大自然科学与工程研究理事会;
关键词
globular clusters : individual (M3; M4; M5; M9; M68; M92; M107); stars : fundamental parameters; stars : horizontal-branch; stars : variables : other (RR Lyrae);
D O I
10.1086/311981
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An examination of the period-V amplitude relation for RRab stars (fundamental mode pulsators) with "normal" light curves in the Oosterhoff type I clusters M3 and M107 and in the Oosterhoff type II clusters M9 and M68 reveals that the V amplitude for a given period is not a function of metal abundance. Rather, it is a function of the Oosterhoff type. This result is confirmed by published observations of RRab stars in M4, M5, and M92. A method devised by Jurcsik & Kovacs has been used to determine whether the light curve of an RRab star is "normal" or "peculiar." Although M3 is considered to belong to the Oosterhoff type I group, it has three bright RRab stars that seem to fit the period-amplitude relation for Oosterhoff type II RRab stars. There is evidence that these bright stars are in a more advanced evolutionary state than the other RRab stars in M3, thus leading to the conclusion that the Oosterhoff dichotomy is due to evolution. Our result gives support to the Lee, Demarque, & Zinn hypothesis that most RR Lyrae variables in Oosterhoff type I clusters are zero-age horizontal branch (ZAHB) objects, while those in the Oosterhoff type II clusters are more evolved. This may have important implications for the derived ages of Oosterhoff type II clusters. If their RR Lyrae variables have all evolved away from the ZAHB, then their ages have been overestimated in studies that assume they are ZAHB objects.
引用
收藏
页码:L85 / L88
页数:4
相关论文
共 30 条
[1]   STUDIES OF RR LYRAE VARIABLE-STARS IN UNUSUAL GLOBULAR CLUSTER OMEGA CENTAURI .1. SPECTROSCOPIC OBSERVATIONS [J].
BUTLER, D ;
DICKENS, RJ ;
EPPS, E .
ASTROPHYSICAL JOURNAL, 1978, 225 (01) :148-164
[2]   BV PHOTOMETRY OF RR LYRAE VARIABLES IN THE GLOBULAR-CLUSTER M92 [J].
CARNEY, BW ;
STORM, J ;
TRAMMELL, SR ;
JONES, RV .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1992, 104 (671) :44-56
[3]   Globular cluster ages and the formation of the galactic halo [J].
Chaboyer, B ;
Demarque, P ;
Sarajedini, A .
ASTROPHYSICAL JOURNAL, 1996, 459 (02) :558-569
[4]   The structure of the light curves of the RR Lyrae variables in the Oosterhoff type I cluster NGC 6171 [J].
Clement, CM ;
Shelton, I .
ASTRONOMICAL JOURNAL, 1997, 113 (05) :1711-1722
[5]   The mode change of the RR Lyrae variable V79 in M3 [J].
Clement, CM ;
Goranskij, VP .
ASTROPHYSICAL JOURNAL, 1999, 513 (02) :767-774
[6]   Evolution of horizontal-branch stars in globular clusters: The interesting case of V79 in M3 [J].
Clement, CM ;
Hilditch, RW ;
Kaluzny, J ;
Rucinski, SM .
ASTROPHYSICAL JOURNAL, 1997, 489 (01) :L55-L58
[7]  
CLEMENT CM, 1999, UNPUB AJ
[8]   BVRI PHOTOELECTRIC PHOTOMETRY AND RADIAL-VELOCITY DATA FOR 4 RR LYRAE STARS IN THE GLOBULAR-CLUSTER NGC-6121 - THE STRANGE CASE OF V15 [J].
CLEMENTINI, G ;
MERIGHI, R ;
PASQUINI, L ;
CACCIARI, C ;
GOUIFFES, C .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1994, 267 (01) :83-102
[9]   Double-mode RR Lyrae variables in the globular cluster M3 [J].
Corwin, TM ;
Carney, BW ;
Allen, DM .
ASTRONOMICAL JOURNAL, 1999, 117 (03) :1332-1340
[10]   PHOTOMETRY OF RR LYRAE VARIABLES IN GLOBULAR CLUSTER NGC 6171 [J].
DICKENS, RJ .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1970, 22 :249-&