The Extent of NGC 6822 Revealed by Its C Star Population
Author(s) -
B. Letarte,
S. Demers,
P. Battinelli,
W. E. Kunkel
Publication year - 2002
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/338319
Subject(s) - astrophysics , physics , stars , carbon star , astronomy , population , star count , star formation , halo , galaxy , k type main sequence star , t tauri star , demography , sociology
Using the CFH12K camera, we apply the four band photometric technique toidentify 904 carbon stars in an area 28' x 42' centered on NGC 6822. A few Cstars, outside of this area were also discovered with the Las Campanas SwopeTelescope. The NGC 6822 C star population has an average I of 19.26 mag leadingto an average absolute I magnitude of -4.70 mag, a value essentially identical to the mean magnitude obtained forthe C stars in IC 1613. Contrary to stars highlighting the optical image of NGC6822, C stars are seen at large radial distances and trace a huge slightlyelliptical halo which do not coincide with the huge HI cloud surroundingNGC6822. The previously unknown stellar component of NGC 6822 has a exponentialscale length of 3.0' +/- 0.1' and can be traced to five scale lengths. The C/Mratio of NGC 6822 is evaluated to br 1.0 +/- 0.2.Comment: accepted, to be published in A
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