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Paper: Blue Variables from the MOA Database
Volume: 203, The Impact of Large-Scale Surveys on Pulsating Star Research, IAU Colloquium 176
Page: 80
Authors: Noda, S.; Takeuti, M.; 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: A large database of CCD photometry for 1.4 million stars towards both the LMC and the SMC, which has been established by the MOA project, is a useful resource to study variable stars. In our preliminary study, variables identified as β Lyrae type stars and Herbig Ae/Be stars have been found amongst blue stars.
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