Observational properties of red variables in the LMC

Details Observational properties of red variables in the LMC Observational properties of red variables in the LMC

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..310..332t&link_type=abstract

Variable Stars in the Local Group, IAU Colloquium 193, Proceedings of the conference held 6-11 July, 2003 at Christchurch, New Z

Astronomy and Astrophysics

Astronomy

Scientific paper

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 color magnitude diagrams based on the MOA red band, Rm, and KS constructed for the sequences, form a single strip with small successive shifts.

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