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Blue Variables from the MOA Database

Published online by Cambridge University Press:  12 April 2016

Sachiyo Noda ,
Mine Takeuti ,
I. A. Bond ,
N. J. Rattenbury ,
F. Abe ,
B. S. Carter ,
R. J. Dodd ,
J. B. Hearnshaw ,
M. Honda  and
J. Jugaku
...Show all authors
Sachiyo Noda
Affiliation:
Solar-Terrestrial Environment Laboratory, Nagoya University, Chikusa, Nagoya 464-8601, Japan
Mine Takeuti
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan

Abstract

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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.

Type
Part 1. Large Scale Surveys: Present and Future
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 80 - 81
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Abe, F., Allen, W., Banks, T., et al. (The MOA Group) 1997, in Variable Stars and the Astrophysical Returns of the Microlensing Surveys, ed. Ferlet, R., Maillard, J.-P., & Raban, B. (Gif-sur-Yvette: Editions Frontières), 75 Google Scholar
Hearnshaw, J.B., Bond, I.A., Rattenbury, N.J., et al. (The MOA Group) 2000, IAU Coll. 176, in these proceedings, p. 31 Google Scholar
Muraki, Y., Sumi, T., Abe, F., et al. (The MOA Group) 1999, Prog. Theor. Phys. Suppl., No. 133, 233 Google Scholar