2010
DOI: 10.1017/s1743921311023076
|View full text |Cite
|
Sign up to set email alerts
|

Asymptotic Giant Branch Variables in NGC 6822

Abstract: Abstract. 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.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals

citations
Cited by 0 publications
references
References 9 publications
0
0
0
Order By: Relevance

No citations

Set email alert for when this publication receives citations?