No CrossRef data available.
Article contents
Variable stars in M31 from the MEGA survey
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The MEGA microlensing survey is introduced and several topics about variable stars in M31 are discussed. An adopted model population of semiregular (SR) variable stars is presented, and the efficiency to recover these stars in M31 in a specific example MEGA dataset is predicted. The period-flux amplitude relation of the SRs discovered by MEGA could be used to measure the inclination of the M31 disk.
- Type
- Part 2. What variable stars tell us about the Local Group, including the distance scale
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 65 - 69
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
Alves, D.R.
et al. 2003a, in ESO Astrophysics Symposia, Towards an International Virtual Observatory, eds. Gorski, K. & Quinn, P. (Berlin: Springer-Verlag), in pressGoogle Scholar
Alves, D.R.
et al. 2003b, in ASP Conf. Ser., Vol. 296, New Horizons in Globular Cluster Astronomy, eds. Piotto, G., Meylan, G., Djorgovski, G. & Riello, M., (San Francisco: ASP), in pressGoogle Scholar
Kaufman, L.
Rousseeuw, P.
1990, “Finding Groups in Data,” (Wiley-Interscience, New York)Google Scholar
You have
Access