Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pabei..11..135y&link_type=abstract
Prog. Astron., Vol. 11, No. 2, p. 135 - 145
Astronomy and Astrophysics
Astronomy
Post-Agb Stars: Stellar Evolution, Post-Agb Stars: Circumstellar Shells
Scientific paper
The evolution characters of post-AGB stars are reviewed. There is a lot of dust in their circumstellar envelopes. There is also a lot of molecules in their circumstellar envelopes, for example CO molecules, OH, H2O, and SiO maser molecules. The evolution characters of post-AGB stars often appear to be constant luminosity, and great increase of their surface temperature.
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