Abundance gradient in Local Group galaxies using Asymptotic Giant Branch stars

Details Abundance gradient in Local Group galaxies using Asymptotic Giant Branch stars Abundance gradient in Local Group galaxies using Asymptotic Giant Branch stars

2004-07-19

arxiv.org/abs/astro-ph/0407397v1

Astronomy and Astrophysics

Astrophysics

5 pages, 4 figures, Contributed talk to the ESO Workshop: "Planetary Nebulae beyond the Milky Way", held at ESO-Garching (Germ

Scientific paper

Simultaneous IJKs observations allow us to statistically select AGB stars,
both M and C type, from RGB and younger or foreground stars in nearby galaxies.
Regions of different metallicity identified from the distribution of the C/M
ratio show a considerable variation across the surface of the Magellanic Clouds
and NGC 6822.

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