Volume 414, Number 1, January IV 2004
|Page(s)||211 - 221|
|Section||Interstellar and circumstellar matter|
|Published online||12 January 2004|
Departamento de Astronomia, IAG/USP, C.P. 3386, 01060-970 São Paulo – SP, Brasil e-mail: firstname.lastname@example.org; email@example.com
Corresponding author: A. V. Escudero, firstname.lastname@example.org
Accepted: 29 September 2003
New observations and derived chemical abundances are reported for a sample of 57 bulge planetary nebulae (PN). Together with our previous results, a total of over a hundred objects have been analyzed, which constitute one of the largest samples of bulge nebulae studied under homogeneous conditions, including equipment and reduction procedures. In general, our data show a good agreement with some recent results in the literature, in the sense that the average abundances of bulge PN are similar to those from disk objects, however showing a larger dispersion.
Key words: planetary nebulae: general / galaxies: bulges / techniques: spectroscopic
© ESO, 2004
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