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Observational properties of red variables in the LMC

Published online by Cambridge University Press:  12 April 2016

M. Takeuti ,
S. Noda ,
F. Abe ,
I.A. Bond ,
R.J. Dodd ,
J.B. Hearnshaw ,
M. Honda ,
M. Honma ,
J. Jugaku  and
Y. Kan-ya
...Show all authors
M. Takeuti
Affiliation:
Astronomical Institute, Tohoku University, Sendai 980-8578, Japan
S. Noda
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan Astronomical Data Analysis Center, National Astronomical Observatory, Japan
F. Abe
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
I.A. Bond
Affiliation:
Institute of Astronomy, University of Edinburgh, Royal Observatory, UK
R.J. Dodd
Affiliation:
Department of Physics, University of Auckland, New Zealand Carter National Observatory, New Zealand School of Chemical and Physical Sciences, Victoria University, New Zealand
J.B. Hearnshaw
Affiliation:
Department of Physics and Astronomy, University of Canterbury, New Zealand
M. Honda
Affiliation:
Institute for Cosmic Ray Research, University of Tokyo, Japan
M. Honma
Affiliation:
VERA Project Office, National Astronomical Observatory, Japan
J. Jugaku
Affiliation:
Institute for Civilization, Tokai University, Japan
Y. Kan-ya
Affiliation:
VERA Project Office, National Astronomical Observatory, Japan
Y. Kato
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
P.M. Kilmartin
Affiliation:
Department of Physics, University of Auckland, New Zealand Department of Physics and Astronomy, University of Canterbury, New Zealand
Y. Matsubara
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
K. Masuda
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
Y. Muraki
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
T. Nakamura
Affiliation:
Department of Physics, Kyoto University, Japan
K. Ohnishi
Affiliation:
Nagano National College of Technology, Japan
M. Reid
Affiliation:
School of Chemical and Physical Sciences, Victoria University, New Zealand
N.J. Rattenbury
Affiliation:
Department of Physics, University of Auckland, New Zealand
To. Saito
Affiliation:
Tokyo Metropolitan College of Aeronautics, Japan
Y. Saito
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
H. Sato
Affiliation:
Research Institute of Fundamental Physics, Kyoto University, Japan
M. Sekiguchi
Affiliation:
Institute for Cosmic Ray Research, University of Tokyo, Japan
J. Skuljan
Affiliation:
Department of Physics and Astronomy, University of Canterbury, New Zealand
D.J. Sullivan
Affiliation:
School of Chemical and Physical Sciences, Victoria University, New Zealand
T. Sumi
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan Department of Astrophysical Science, Princeton University, USA
R. Yamada
Affiliation:
Solar-Terrestrial Environment Lab., Nagoya University, Nagoya 464-8601, Japan
T. Yanagisawa
Affiliation:
National Aeronautical Laboratory of Japan, Space Research Technology Center, Japan
P.C.M. Yock
Affiliation:
Department of Physics, University of Auckland, New Zealand
M. Yoshizawa
Affiliation:
Department of Fundamental Astrometry, National Astronomical Observatory, Japan

Abstract

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More than 4000 stars observed in both MOA and DENIS projects showing periodic or quasi-periodic light curves are studied. Almost all Mira stars are located on the classical period-luminosity relation, and the multiplicity of the period-luminosity relation is confirmed for small-amplitude stars. The colour-magnitude diagrams based on the MOA red band, Rm, and Ks constructed for the sequences, form a single strip with small successive shifts.

Type
Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 332 - 335
Copyright
Copyright © Astronomical Society of the Pacific 2004

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