Classification of ISO SWS 01 spectra of proto-planetary nebulae: a
search for precursors of planetary nebulae with [WR] central stars.
Szczerba R., Stasinska G., Siodmiak N, Gorny S.K.
2003, in Proceedings of the Symposium
"Exploiting the ISO Data Archive - Infrared Astronomy in the Interenet Age", Eds.C. Gry, S. Peschke, J. Matagne, P. Garcia-Lario, R. Lorente, & A. Salama, ESA SP-511, 149
Abstract:
- We have analyzed ISO SWS 01 observations for 61 proto-planetary
nebulae candidates and classified their spectra according to their
dominant chemistry. On the basis of our classification and the more general
classification of SWS 01 spectra by Kraemer et al.(2002) we discuss the
connection between proto-planetary nebulae candidates and planetary
nebulae, with emphasis on possible precursors of planetary nebulae
with [WR] central stars.
Gzipped PostScript version of this paper is available: poster_Siguenza.ps.gz
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