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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S283(7), p. 404-405, 2011

DOI: 10.1017/s1743921312011647

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Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe)

Journal article published in 2011 by Graziela R. Keller, Luciana Bianchi ORCID, James E. Herald, Walter J. Maciel
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe present comprehensive grids of model spectra from far-UV to IR, covering the parameter space of [WC] (Keller et al. 2011) and PG1159 stars. Models are calculated with the CMFGEN code, accounting for non-LTE, line blanketing, wind, clumping, and including ions previously neglected. The grids are available at http://dolomiti.pha.jhu.edu/planetarynebulae.html. We used them to analyse UV and far-UV spectra of NGC6905's and NGC5189's central stars.

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