000004591 001__ 4591
000004591 005__ 20200122112004.0
000004591 037__ $$aPOSTER-2020-0020
000004591 100__ $$aWiegert, Joachim
000004591 245__ $$aExploring dust mass and dust properties of nearby AGB stars 
000004591 260__ $$c2018
000004591 269__ $$c2018-08-20
000004591 520__ $$aLow and intermediate mass stars evolve to the asymptotic red giant branch (AGB) late in their lives. These are surrounded by a circumstellar envelope (CSE) filled with gas and dust. The dust is formed close to the star at sublimation radii and is pushed away by the stellar wind. The dust in turn pushes gases from the envelope into the interstellar medium, thus enriching it with metals. This poster summary is a general description of the next piece of a larger project, whereas the first half has been published by Nicolaes et al. (2018). We now aim to use radiative transfer simulations to model spectral energy distributions (SED) of dust and fit them to far-infrared observations for the same 40 sources. We will use 2D and 3D simulations and models containing several dust species simultaneously.
000004591 536__ $$aBR/$$c143/$$fA2/STARLAB
000004591 594__ $$aNO
000004591 700__ $$aGroenewegen, Martin
000004591 700__ $$aSTARLAB, Consortium
000004591 773__ $$tIAU Symposium 343, Vienna
000004591 8560_ $$fmartin.groenewegen@observatoire.be
000004591 980__ $$aCPOSTER