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Long Period Variables in the Magellanic Clouds: the OGLE/MACHO/2MASS/DENIS view

Published online by Cambridge University Press:  12 April 2016

Martin Groenewegen*
Affiliation:
Instituut voor Sterrenkunde, Celestijnenlaan 200B, B-3001 Leuven, Belgium

Abstract

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I present a brief analysis of K-band period-luminosity relations for AGB stars in the SMC based on OGLE, 2MASS and DENIS data. I also present, for a selected sample of SMC and LMC stars, a comparison between the analysis of respective MACHO and OGLE data and a method to combine the data from the two surveys.

Type
Part 2. What variable stars tell us about the Local Group, including the distance scale
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Cioni, M.-R. et al. 2001 A&A 377, 495 Google Scholar
Cioni, M.-R.L. et al. 2003 A&A, 406, 51 Google Scholar
Ita, Y. et al. 2003, preprintGoogle Scholar
Kiss, L.L., Bedding, T. 2003 MNRAS, 343, L79 CrossRefGoogle Scholar
Lebzelter, T., Schuiteis, M., Melchior, A.L. 2002 A&A, 393, 573 Google Scholar
Noda, S. et al. 2002 MNRAS 330, 137 Google Scholar
Wood, P.R. et al. 1999, in IAU Symposium 191, Asymptotic Giant Branch Stars, eds. Le Bertre, T., Lebre, A. & Waelkens, C., (ASP, San Francisco), 151 Google Scholar
Wood, P.R. 2000 PASA, 17, 18 CrossRefGoogle Scholar