Winds of M-type AGB stars driven by micron-sized grains

2008227 citationsJournal Articlebronze Open Access

Authors

Abstract

Context. In view of the recent problem regarding the dynamical modelling of winds of M-type AGB stars (insufficient radiation pressure on silicate grains), some of the basic assumptions of these models need to be re-evaluated critically.

Topics & Keywords

Astrophysics and Star Formation Studies Astro and Planetary Science Stellar, planetary, and galactic studies

UN Sustainable Development Goals

Climate action

Publication Details

Published in: Astronomy and Astrophysics

Volume 491, Issue 2, pp. L1-L4

DOI: 10.1051/0004-6361:200810641

Field-Weighted Citation Impact: 7.09