Modelling planetary nebulae with emission-line nuclei

Details Modelling planetary nebulae with emission-line nuclei Modelling planetary nebulae with emission-line nuclei

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..323a&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

We discuss a sample of 101 planetary nebulae (PNe) analyzed with the
Torun model. We compare the characteristics of [WR] and wels (weak
emission line stars) PNe with those with non-emission line central
stars.

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