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The Centre of the LMC Bar – Analysis of HST Data
Published online by Cambridge University Press: 25 May 2016
Abstract
We used the HST to obtain high resolution images of the LMC Bar centre. Through careful data analysis, taking into account cleaning, dithering and crowded field decomposition, we show that accurate uvby photometry can be achieved for F dwarfs, reaching stars around the lower turn-off region, as faint as V=22.
- Type
- Part 5. Stellar Populations and Surveys
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 359 - 360
- Copyright
- Copyright © Astronomical Society of the Pacific 1999