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Cepheids and LPVs in and around Magellanic Cloud Clusters
Published online by Cambridge University Press: 12 April 2016
Abstract
V and I band CCD photometry of the young clusters NGC 330 (SMC), NGC 1850, NGC 2058 and NGC 2065 (LMC) has been used to find variable stars in and around the clusters. The variables detected are mostly Cepheids and long-period variables (LPVs). Here we outline some results of these studies.
- Type
- Part 2. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 383 - 384
- Copyright
- Copyright © Astronomical Society of the Pacific 1995