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X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
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DTSTART:20180325T010000
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DTSTART:20181028T010000
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DTSTART:20190331T010000
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DTSTART:20191027T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20190926T114500
DTEND;TZID=Europe/Rome:20190926T124500
DTSTAMP:20260508T131018
CREATED:20190612T065845Z
LAST-MODIFIED:20190925T064343Z
UID:6291-1569498300-1569501900@www.oa-roma.inaf.it
SUMMARY:Modeling stellar winds on the asymptotic giant branch accurately
DESCRIPTION:I present the latest progress on our ongoing work with our state-of-the-art\nmodels of stellar winds of asymptotic giant branch stars. I will both depict\nfeatures and assumptions of our model code T-800 and show some of the results\nthat set our work apart; because\, results are in several a case drastically\ndifferent from earlier results. In particular\, I focus on effects of\ngas-to-dust drift and higher-than-before spatial resolution.
URL:https://www.oa-roma.inaf.it/event/chris-sandin-colloquium/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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