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PNe in NGC 300: Their abundances and chemical gradients†

Published online by Cambridge University Press:  30 August 2012

Miiriam Peña ,
Grazyna Stasinska ,
Fabio Bresolin  and
Yiannis Tsamis
Miiriam Peña
Affiliation:
Instituto de Astronomia, UNAM. Apdo. Postal 70264, 04510 Mexico D.F., email: miriam@astro.unam.mx
Grazyna Stasinska
Affiliation:
LUTH, Observatoire de Paris, 5 Place Jules Janssen 92190 Meudon, France email: grazyna.stasinska@obspm.fr
Fabio Bresolin
Affiliation:
Institute for Astronomy, 2680 Woodlan Drive, Honolulu, Hi 96822, USA email: bresolin@ifa.hawaii.edu
Yiannis Tsamis
Affiliation:
ESO, Karl-Schwarzchild Str. 2, D-85748 Garching bei Munchen, Germany email: ytsamis@eso.org
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Abstract

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Spectrophotometric data of a number of planetary nebulae and compact HII regions of NGC 300 have been obtained with the FORS 2 spectrograph of the VLT. We present a preliminary analysis of such data.

Keywords

Galaxies: individual (NGC 300)planetary nebulae: generalISM: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 263 - 266
Copyright
Copyright © International Astronomical Union 2012

References

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