Binary (Post) AGB evolution

Details Binary (Post) AGB evolution Binary (Post) AGB evolution

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.275..159v&link_type=abstract

Astrophysics and Space Science, v. 275, Issue 1/2, p. 159-167 (2001).

Astronomy and Astrophysics

Astrophysics

12

Scientific paper

In this contribution the observational characteristics of F to G type post-AGB stars, showing both O-rich and C-rich circumstellar chemistry, are reviewed. It turns out that binarity and the presence of a stable circumbinary dusty disc are fundamental properties of these objects. The possible common origin of the mixed chemistry observed in these systems and in IR-bright [WC] stars is discussed.

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