Post-AGB Stars

By H. Winckel. 2003

338 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/ea57fa38963b798adce1712be824cf949645f55b

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In Astronomy and Astrophysics

Citations in the corpus

Keplerian discs around post-AGB stars: a common phenomenon? (2006, background): “Other examples exist and there is substantial observational evidence that the systems are all likely surrounded by a circumstellar orbiting disc (Van Winckel 2003).”
Evolution of Asymptotic Giant Branch Stars (2005, background): “The colors indicating convection zones, layers with H-shell ashes and the region of the 13C pocket match those in Figure 5. post-AGB stars and their observational implications for the s-process (van Winckel 2003).”
Stellar Models and Yields of Asymptotic Giant Branch Stars (2007, background): “After the outer envelope has been ejected the stars evolve through the brief post-AGB and planetary nebula (PN) phases of the Hertzsprung–Russell diagram (van Winckel 2003).”
Dawes Review 6: The Impact of Companions on Stellar Evolution (2016, background): “…cores of RGB stars Drechsel et al. 2001 Post-CE central stars of PN CE interaction during the AGB Miszalski et al. 2009a Post-AGB binaries Post-AGB+MS binaries; P∼100–1 000 days with circumbinary disks Van Winckel 2003 FS Canis Majoris Hot+cool close binaries exhibiting the B[e] phenomenon (?)”
Formation and dynamical evolution of multiple stellar generations in globular clusters (2008, background): “…to M −10 core, so that, while it is >10000yr at the core masses of typical planetary nebula nuclei (0.6M⊙), it is only a few hundred years for the core masses 1.0–1.3 M⊙ that are remnants of the possible progenitors of the SG we are considering (see also Van Winckel 2003, for a review).”
The Progenitors of Type Ia Supernovae (2012, background): “This assumption has been widely used to explain many phenomena related to giant star evolution in binaries (e.g. Han, 1998; van Winckel, 2003).”