<html><head><meta http-equiv="content-type" content="text/html; charset=utf-8"></head><body dir="auto">Welcome!<div><br><div>Angela & Jorrit </div><div><br>On 2 May 2018, at 10:04, Angela Adamo <<a href="mailto:angela.adamo@astro.su.se">angela.adamo@astro.su.se</a>> wrote:<br><br></div><blockquote type="cite"><div>
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Dear all,
<div class="">welcome to our weekly appointment. </div>
<div class="">The speaker of this week is Dr. Sara Bladh, from the University of Uppsala.</div>
<div class="">Sara is an expert in modelling radiation-driven winds in late type stars.</div>
<div class=""><br class="">
</div>
<div class="">Title: The evolution of DARWIN - the current status of wind models for AGB stars</div>
<br class="">
Abstract: Asymptotic giant branch (AGB) stars are luminous, cool giants with substantial mass loss. Dust formed in the stellar atmospheres plays a key role for the mass-loss mechanism: radial pulsations of the surface layers of the stars levitate material to
distances where dust can form, which then is accelerated outward by radiation pressure. AGB stars are significant dust donors in the universe, feeding newly produced elements into the surrounding interstellar medium in the form of gas and dust through these
stellar winds.<br class="">
<br class="">
To model these dense outflows we use the DARWIN (Dynamic Atmosphere and Radiation-driven Wind models based on Implicit Numerics) code. The mass-loss process is modelled from first principles, with frequency-dependent radiation-hydrodynamics, and dust growth
and evaporation. The DARWIN models have successfully been able produce outflows with dynamical and photometric properties compatible with observations, for both C-type and M-type AGB stars (e.g. Eriksson et al. 2014, Bladh et al. 2015). In this talk I will
present the recent development in the DARWIN wind models: I will show results from a new large grid of M-type AGB star models, spanning a wide range in effective temperature, mass and lumiosity, as well as results from models for C-type AGB stars at low metallicities,
compatible to those in LMC and SMC.<br class="">
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</div>
<div class=""><br class="">
</div>
<div class="">Our seminar agends is available both on the albanova webpage <a href="https://www.albanova.se/events/seminars/" class="">
https://www.albanova.se/events/seminars/</a> and on our department webpage <a href="https://www.astro.su.se" class="">https://www.astro.su.se</a> ("upcoming events”/“kommande händelser”)</div>
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</div>
<div class="">Kind regards,</div>
<div class="">Angela & Jorrit</div>
<div class=""><br class="">
</div>
<div class="">-------------------------------------------------------<br class="">
Angela Adamo <br class="">
<br class="">
Department of Astronomy<br class="">
Stockholm University and Oskar Klein Centre<br class="">
SE-10691 Stockholm - Sweden<br class="">
tel: +46 (0)8 5537 8556 <br class="">
email: <a href="mailto:angela.adamo@astro.su.se" class="">angela.adamo@astro.su.se</a><br class="">
<a href="http://ttt.astro.su.se/~adamo" class="">http://ttt.astro.su.se/~adamo</a><br class="">
------------------------------------------------------- </div>
<br class="">
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