TY  - GEN
A1  - Todt, Helge Tobias
A1  - Peña, Miriam
A1  - Zühlke, Julia
A1  - Oskinova, Lida
A1  - Hamann, Wolf-Rainer
A1  - Gräfener, Götz
T1  - Weak emission line central stars of planetary nebulae
T2  - Planetary Nebulae: an Eye to the Future
N2  - To understand the evolution and morphology of planetary nebulae, a detailed knowledge of their central stars is required. Central stars that exhibit emission lines in their spectra, indicating stellar mass-loss allow to study the evolution of planetary nebulae in action. Emission line central stars constitute about 10 % of all central stars. Half of them are practically hydrogen-free Wolf-Rayet type central stars of the carbon sequence, [WC], that show strong emission lines of carbon and oxygen in their spectra. In this contribution we address the weak emission-lines central stars (wels). These stars are poorly analyzed and their hydrogen content is mostly unknown. We obtained optical spectra, that include the important Balmer lines of hydrogen, for four weak emission line central stars. We present the results of our analysis, provide spectral classification and discuss possible explanations for their formation and evolution.
T3  - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 462 
KW  - stars: AGB and post-AGB
KW  - stars: Wolf-Rayet
KW  - stars: abundances
Y1  - 2018
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-413775
ER  -