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Observational properties of red variables in the LMC
Published online by Cambridge University Press: 12 April 2016
Abstract
More than 4000 stars observed in both MOA and DENIS projects showing periodic or quasi-periodic light curves are studied. Almost all Mira stars are located on the classical period-luminosity relation, and the multiplicity of the period-luminosity relation is confirmed for small-amplitude stars. The colour-magnitude diagrams based on the MOA red band, Rm, and Ks constructed for the sequences, form a single strip with small successive shifts.
- Type
- Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 332 - 335
- Copyright
- Copyright © Astronomical Society of the Pacific 2004