Stellar populations in the Magellanic Clouds: looking through the dust
arXiv:astro-ph/0702020 · doi:10.1017/S1743921307008320
Abstract
We present the first results of our study of stellar populations in the Large and Small Magellanic Clouds based on multi-band WFPC2 observations of "random" fields taken as part of the "pure parallel" programme carried out with the HST as a service to the community.
Two pages, one figure, to appear in the proceedings of IAU Symposium 241 "Stellar Populations as Building Blocks of Galaxies", eds. A. Vazdekis and R. Peletier
References in corpus (5)
- The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map
- Young Stellar Populations Around SN1987A
- Accurate Stellar Population Studies from Multiband Photometric Observations
- Low-Mass Pre-Main Sequence Stars in the Large Magellanic Cloud - III: Accretion Rates from HST-WFPC2 Observations
- The WFPC2 Archival Parallels Project