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AGB variables in globular clusters
Published online by Cambridge University Press: 12 April 2016
Abstract
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
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 144 - 148
- Copyright
- Copyright © Astronomical Society of the Pacific 2004