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AGB variables in globular clusters

Published online by Cambridge University Press:  12 April 2016

T. Lebzelter
Affiliation:
University of Vienna, Türkenschanzstrasse 17, A1180 Vienna, Austria
P. Wood
Affiliation:
RSAA, Australian National University, Canberra, Australia
K.H. Hinkle
Affiliation:
NOAO, Tucson, AZ 85726, USA
R. Joyce
Affiliation:
NOAO, Tucson, AZ 85726, USA
F. Fekel
Affiliation:
Tennessee State University, Nashville, TN 37203-3401, USA
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Abstract

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With a large number of newly detected red variables in globular clusters we construct a log P – K diagram of these stars and compare it with findings from the LMC. We show the existence of a relation between the location in log P – K diagram and the velocity amplitude in the near infrared.

Type
Part 3. Variable stars as tracers of different stellar populations – galactic and globular clusters, LMC/SMC and Local Group galaxies
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Alard, C. 2000 A&AS, 144, 363 Google Scholar
Clement, C.M., et al. 2001 AJ, 122, 2587 CrossRefGoogle Scholar
Höfner, S., et al. 2003 A&A, 399, 589 Google Scholar
Lebzelter, T., Hinkle, K.H. 2002, in ASP Conf. Ser. Vol. 259, Radial and non-radial pulsations as probes of stellar physics, ed. Aerts, C., Bedding, T.R. & Christensen-Dalsgaard, J.C. (San Francisco ASP), 556 Google Scholar
Pritzl, B.J., et al. 2002 AJ, 124, 949 CrossRefGoogle Scholar
Rosenberg, A., et al. 2000 A&AS, 144, 5 Google Scholar
Wood, P.R. 2000 PASA, 17, 18 CrossRefGoogle Scholar
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