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Red Variables from the MOA Database

Published online by Cambridge University Press:  12 April 2016

Mine Takeuti ,
Sachiyo Noda ,
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
Mine Takeuti
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan
Sachiyo Noda
Affiliation:
Solar-Terrestrial Environment Laboratory, Nagoya University, Chikusa, Nagoya 464-8601, Japan
K. Masuda
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan
P. C. M. Yock
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan

Abstract

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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
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 120 - 121
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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