Issue |
EAS Publications Series
Volume 48, 2011
CRAL-2010 A Universe of Dwarf Galaxies
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|
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Page(s) | 63 - 64 | |
Section | Star Formation History and Chemical Enrichment | |
DOI | https://doi.org/10.1051/eas/1148011 | |
Published online | 11 July 2011 |
A Universe of Dwarf Galaxies
M. Koleva, Ph. Prugniel and I. Vauglin (eds)
EAS Publications Series, 48 (2011) 63–64
M. Koleva, Ph. Prugniel and I. Vauglin (eds)
EAS Publications Series, 48 (2011) 63–64
NGC 6822: SFH of its Intermediate-Age Population
1 Université de Montréal
2 INAF, OAR
We have monitored, during four years, a 32′× 32′ area of the Local Group dwarf galaxy NGC 6822. Observations lead to the discovery of 30 Miras and 24 semi-regular and irregular variables. When relating the periods of Miras to their age, we find a continuous star formation during the last 3 Gyr. This result is basically consistent with the hypothesis that the intermediate-age population of NGC 6822 was born following the “polar ring” formation.
© EAS, EDP Sciences, 2011