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

Published online by Cambridge University Press:  30 August 2012

Graziela R. Keller
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Cidade Universitária, São Paulo/SP, Brazil. Email: [email protected]
Luciana Bianchi
Affiliation:
Department of Physics and Astronomy, The Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA.
James E. Herald
Affiliation:
Department of Physics and Astronomy, The Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA.
Walter J. Maciel
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Cidade Universitária, São Paulo/SP, Brazil. Email: [email protected]
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Abstract

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We 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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Hillier, D. J. & Miller, D. L. 1998, ApJ, 496, 407 CrossRefGoogle Scholar
Keller, G. R., Herald, J. E., Bianchi, L., Maciel, W. J., & Bohlin, R. C 2011, MNRAS, in pressGoogle Scholar
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