2002/12/10 by R. Szczerba, G. Stasi{ń}ska, Szczerba, R. +5
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0212239
4 pages, 7 figures, Proceedings of the Symposium "Exploiting the ISO Data Archive - Infrared Astronomy in the Internet Age"
arxiv created 2002/12/10 · arxiv updated 2016/08/16
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.