Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-06-20T15:09:18.694Z Has data issue: false hasContentIssue false
  • English
  • Français

Integral stellar-nebular model of NGC 7009

Published online by Cambridge University Press:  30 August 2012

Celia R. Fierro ,
Antonio Peimbert ,
Leonid Georgiev ,
Christophe Morisset  and
Anabel Arrieta
Celia R. Fierro
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México D.F, C.P. 04510, México email: crfierro@astro.unam.mx, antonio@astroscu.unam.mx, georgiev@astro.unam.mx, chris.morisset@gmail.com, and anabel.arrieta@uia.mx
Antonio Peimbert
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México D.F, C.P. 04510, México email: crfierro@astro.unam.mx, antonio@astroscu.unam.mx, georgiev@astro.unam.mx, chris.morisset@gmail.com, and anabel.arrieta@uia.mx
Leonid Georgiev
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México D.F, C.P. 04510, México email: crfierro@astro.unam.mx, antonio@astroscu.unam.mx, georgiev@astro.unam.mx, chris.morisset@gmail.com, and anabel.arrieta@uia.mx
Christophe Morisset
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México D.F, C.P. 04510, México email: crfierro@astro.unam.mx, antonio@astroscu.unam.mx, georgiev@astro.unam.mx, chris.morisset@gmail.com, and anabel.arrieta@uia.mx Instituto de Astrofísica de Canarias, E-38200, La Laguna, Tenerife, Spain.
Anabel Arrieta
Affiliation:
Universidad Iberoamericana, Departamento de Física y Matemáticas, Avenida Prolongacion Paseo de la Reforma 880, Lomas de Santa Fe, CP 01210, México, DF, México
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We developed a self-consistent stellar-nebular model for NGC 7009. This model reproduces the available observations ranging from optical to UV. The combined approach to the modeling process produces more constraints and thus more trustworty results. After obtaining the model, we perform a comparative study of the chemical composition of He, N, O, Ne, Cl, and S in the nebula and its central star. Concluding that the stellar composition agrees with the nebular composition with t2 ≠ 0.00.

Keywords

stars: abundancesstars: atmospheresstars: fundamental parametersstars: rotationstars: windsoutflowsISM: abundancesplanetary nebulae: individual (NGC 7009)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 356 - 357
Copyright
Copyright © International Astronomical Union 2012

References

Vassiliadis, E. & Wood, P. R. 1994, ApJS, 92, 125 CrossRefGoogle Scholar
Hiller, D. J. & Miller, D. 1998, ApJ, 496, 407 Google Scholar
Ferland, G. J., Korista, K. T., Verner, D. A., et al. 1998, PASP, 110, 761 CrossRefGoogle Scholar