Abundances of non-type I PNe in LMC Virtual Observatory Resource

Authors
  1. de Freitas Pacheco J.A.
  2. Costa R.D.D.
  3. Maciel W.J.
  4. Published by
    CDS
Abstract

Spectroscopic observations, plasma diagnostics and chemical composition of 15 non-type I planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) are reported. Abundances of He, O, N, S, and Ar are determined and compared with recently obtained data for nebulae both in the Magellanic Clouds and in the Galaxy.

Keywords
  1. planetary-nebulae
  2. spectroscopy
  3. chemical-abundances
Bibliographic source Bibcode
1993A&A...279..567D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/279/567
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/279/567
Document Object Identifer DOI
doi:10.26093/cds/vizier.32790567

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History

2001-07-15T21:56:27Z
Resource record created
2001-07-15T21:56:27Z
Created
2018-01-10T11:47:38Z
Updated

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr