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Record Details

Record 30 of 767
The RR Lyrae variables in the globular cluster M68
External Online Source: doi:10.1086/172910
Author and Affiliation:
Clement, Christine M.(NASA, Washington, DC, United States)
Ferance, Stephen(David Dunlap Observatory, Toronto, Canada)
Simon, Norman R.(Nebraska Univ., Lincoln, United States)
Abstract: New observations, made with the Helen Sawyer Hogg telescope at Las Campanas, have been analyzed in a search for double-mode pulsators (RRd stars) in the metal-poor globular cluster, Messier 68. Of the 30 stars studied, nine have been identified as RRd stars; V33, which exhibited the characteristics of an RRd star in 1950, now appears to be an RRc star. Reliable periods and period ratios have been determined for six of the RRd stars. Masses for these RRd stars, calculated from fitting formulas given by Kovacs et al. (1991), range from 0.75 to 0.90 solar mass, depending on the assumed luminosity and metal abundance. These masses are in the same range as those for the RRd stars in M 15, whose RRd sample resembles that of M68 very closely. Fourier parameters determined for the light curves of the M68 variables show that the RRc stars in the two clusters are also very similar. In particular, on the plot of phase parameter phi sub 31 with period, the M15 and M68 RRc samples are virtually indistinguishable. A comparison of the new M68 observations with observations made 40 yr ago shows that the periods of some of the stars have changed, but the 40 yr interval is too short for detecting period changes caused by evolutionary effects.
Publication Date: Jul 20, 1993
Document ID:
19930062318
(Acquired Dec 28, 1995)
Accession Number: 93A46315
Subject Category: ASTROPHYSICS
Document Type: Journal Article
Publication Information: Astrophysical Journal, Part 1; p. p. 183-191.; (ISSN 0004-637X); 412; 1
Publisher Information: United States
Financial Sponsor: NASA; United States
Organization Source: NASA; Washington, DC, United States
Description: 9p; In English
Distribution Limits: Unclassified; Publicly available; Unlimited
Rights: Copyright
NASA Terms: GLOBULAR CLUSTERS; STELLAR OSCILLATIONS; VARIABLE STARS; ABUNDANCE; LIGHT CURVE; METALLICITY; STELLAR LUMINOSITY; STELLAR MASS
Imprint And Other Notes: Astrophysical Journal, Part 1 vol. 412, no. 1 p. 183-191. July 20, 1993
Miscellaneous Notes: Research supported by NSERC and NASA
Availability Source: Other Sources
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