Asymptotic Giant Branch Variables in NGC 6822

Details Asymptotic Giant Branch Variables in NGC 6822 Asymptotic Giant Branch Variables in NGC 6822

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..277..337w&link_type=abstract

Tracing the Ancestry of Galaxies (on the land of our ancestors), Proceedings of the International Astronomical Union, IAU Sympos

Other

Stars: Agb And Post-Agb, Stars: Carbon, Stars: Variables: Other, Galaxies: Individual: Ngc 6822, Galaxies: Stellar Content, (Galaxies:) Local Group

Scientific paper

Multi-epoch JHKS photometry is used to identify large
amplitude variables and to study the AGB population of NGC 6822. 50 Mira
variables, ranging in period from 128 to 998 days, have been identified.
The majority of these are around 1 to 4 Gyr old, but a significantly
younger component is also identified.

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