ON THE [ArIV]/[ArIII] LINE RATIO IN PLANETARY NEBULAE

Authors

  • R. E. Carlos Reyes Universidad de Sao Paulo, Instituto Astronomico e Geofisico, Brazil. Universidad Nacional Mayor de San Marcos, Facultad de Ciencias Físicas, Seminario de Astronomía y Ciencias del Espacio, Lima, Peru
  • F. Elizalde Universidad Nacional Mayor de San Marcos, Facultad de Ciencias Físicas, Seminario de Astronomía y Ciencias del Espacio, Lima, Peru
  • J. E. Steiner Universidad de Sao Paulo, Instituto Astronomico e Geofisico, Brazil. Universidad Nacional Mayor de San Marcos, Facultad de Ciencias Físicas, Seminario de Astronomía y Ciencias del Espacio, Lima, Peru

DOI:

https://doi.org/10.15381/rif.v3i01-02.8615

Keywords:

planetary nebulae, stars, emission lines, spectroscopy, ionization modeling

Abstract

Previous spectroscopic studies of planetary nebulae have shown that the observed [ArIV]/[ArIII] line ratio is not reproduced by photoionization models. We show that this discrepancy disappears if we consider an adequate combination of the filling factor and radial density profile.

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Published

2000-11-30

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Article

How to Cite

ON THE [ArIV]/[ArIII] LINE RATIO IN PLANETARY NEBULAE. (2000). Revista De Investigación De Física, 3(01-02), 48-50. https://doi.org/10.15381/rif.v3i01-02.8615