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X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
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DTSTART:20160327T010000
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DTSTART:20170326T010000
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DTSTART;TZID=Europe/Rome:20171205T114500
DTEND;TZID=Europe/Rome:20171205T124500
DTSTAMP:20260506T231156
CREATED:20170816T120046Z
LAST-MODIFIED:20170816T120046Z
UID:3398-1512474300-1512477900@www.oa-roma.inaf.it
SUMMARY:Mass loss of AGB stars and RSG in the Magellanic Clouds
DESCRIPTION:I will discuss recent work that I am involved in regarding the determination of\nthe mass-loss rates (MLRs)  of a significant sample of Asymptotic Giant Branch stars and\nRed Supergiants in the Magellanic Clouds. This mostly involves modelling the\nspectral energy distributions to obtain dust MLRs\, but we also used ALMA to detect CO emission\nin a few LMC objects. I will also discuss possible ways forward in this field
URL:https://www.oa-roma.inaf.it/event/talk-by-martin-groenewegen/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20171205T114500
DTEND;TZID=Europe/Rome:20171205T124500
DTSTAMP:20260506T231156
CREATED:20170816T120046Z
LAST-MODIFIED:20170816T120046Z
UID:4722-1512474300-1512477900@www.oa-roma.inaf.it
SUMMARY:Mass loss of AGB stars and RSG in the Magellanic Clouds
DESCRIPTION:I will discuss recent work that I am involved in regarding the determination of\nthe mass-loss rates (MLRs)  of a significant sample of Asymptotic Giant Branch stars and\nRed Supergiants in the Magellanic Clouds. This mostly involves modelling the\nspectral energy distributions to obtain dust MLRs\, but we also used ALMA to detect CO emission\nin a few LMC objects. I will also discuss possible ways forward in this field
URL:https://www.oa-roma.inaf.it/event/talk-by-martin-groenewegen-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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