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| Paper: |
Red Variables from the MOA Database |
| Volume: |
203, The Impact of Large-Scale Surveys on Pulsating Star Research, IAU Colloquium 176 |
| Page: |
120 |
| Authors: |
Takeuti, M.; Noda, S.; Bond, I. A.; Rattenbury, N. J.; Abe, F.; Carter, B. S.; Dodd, R. J.; Hearnshaw, J. B.; Honda, M.; Jugaku, J.; Kabe, S.; Kilmartin, P. M.; Masuda, K.; Matsubara, Y.; Muraki, Y.; Nakamura, T.; Reid, M.; Rumsey, N. J.; Saito, To.; Sato, H.; Sekiguchi, M.; Sullivan, D. J.; Sumi, T.; Watase, Y.; Yanagisawa, T.; Yock, P. C. M.; Yoshizawa, M. |
| 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. |
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