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Red Variables from the MOA Database
Published online by Cambridge University Press: 12 April 2016
Abstract
The red variables whose amplitude is larger than 1.3 mag in the MOA database are studied for the LMC. Among 3 196 such stars, 532 stars are likely to be Miras or red semiregular variables. The period–colour relation of these stars is shown.
- Type
- Part 2. Variability of High-Luminosity Stars
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- Copyright © Astronomical Society of the Pacific 2000