Quantitative Spectral Analysis of hot Post-AGB Stars

Details Quantitative Spectral Analysis of hot Post-AGB Stars Quantitative Spectral Analysis of hot Post-AGB Stars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..265..356c&link_type=abstract

Chemical Abundances in the Universe: Connecting First Stars to Planets, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Stars: Agb And Post-Agb - Stars: Abundances - Stars: Evolution

Scientific paper

Post-AGB (PAGB) stars are luminous objects of low and intermediate mass in a final and short stage of evolution in the transition between AGB stars and planetary nebulae (PNe). In this work we present a quantitative spectral analysis of some hot PAGBs based on high resolution spectra. The stellar parameters and chemical composition were obtained from the synthesis of non-LTE spectra.

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