On the Mass-Loss History at the Tip of the AGB

Details On the Mass-Loss History at the Tip of the AGB On the Mass-Loss History at the Tip of the AGB

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..343s&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We demonstrate by means of radiation-hydrodynamics simulations how the
spectral energy distribution (SED) of post-AGB objects depends on the
mass-loss properties during evolution off the tip of the AGB.

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