In:
Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 7, No. S283 ( 2011-07), p. 404-405
Kurzfassung:
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.
Materialart:
Online-Ressource
ISSN:
1743-9213
,
1743-9221
DOI:
10.1017/S1743921312011647
Sprache:
Englisch
Verlag:
Cambridge University Press (CUP)
Publikationsdatum:
2011
ZDB Id:
2170724-8
SSG:
16,12