CHEMICAL ABUNDANCES OF PLANETARY NEBULAE TOWARDS THE GALACTIC ANTICENTER
R. D. D. Costa, M. M. M. Uchida, W.J. Maciel
Astronomy and Astrophysics 423, 199-207 (2004)
In this paper we report new observations and derive chemical
abundances for a sample of 26 planetary nebulae (PN) located in the anticenter
direction. Most of these nebulae are far away objects, located at
galactocentric distances greater than about 8 kpc, so that they are
particularly useful for the determination of the radial gradients at
large distances from the galactic center. A comparison of the present
results with previously determined abundances suggests that the
radial abundance gradients flatten out at distances larger than
about 10 kpc from the center.
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