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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

References

Barthes, D., Luri, X. 2001, A&A, 365, 519 Google Scholar
Bedding, T.R., Zijlstra, A.A. 1998, ApJ, 506, L47 Google Scholar
Feast, M.W., Glass, I.S., Whitelock, P.A., Catchpole, R.M. 1989, MNRAS, 241, 375 Google Scholar
Hearnshaw, J.B., Bond, I.A., Rattenbury, N.J., et al. 2000, in ASP Conf. Ser. Vol. 203, The Impact of Large-scale Surveys on Pulsating Star Research, eds Szabados, L., & Kurtz, D.W. (San Francisco: ASP), 203, 31 Google Scholar
Hughes, S.M.C., Wood, P.R. 1990, AJ, 99, 784 Google Scholar
Lebzelter, T., Schultheis, , Melchior, A.L. 2002, A&A, 393, 573 Google Scholar
Noda, S., Takeuti, M. 2003, in ASSL Vol. 283, Mass-losing Pulsating Stars and Their Circumstellar Matter, ed. Nakada, Y., Honma, M., & Seki, M. (Dordrecht: Kluwer), 27 Google Scholar
Noda, S., Takeuti, M., Abe, F., et al. 2002, MNRAS, 330, 137 Google Scholar
Noda, S., Takeuti, M., Abe, F., et al. 2003, MNRAS, acceptedGoogle Scholar
Rejkuba, M. 2003, A&A, submittedGoogle Scholar
Wood, P.R. 2000, PASA, 17, 18 Google Scholar
Wood, P.R., Alcock, C. Allsman, R.A., et al. 1999, in IAU Symp. 191, Asymptotic Branch Stars, ed. Bertre, T., Lebre, A., & Waelkens, C. (San Francisco: ASP), 151 Google Scholar