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DTSTART;TZID=Europe/Rome:20180911T114500
DTEND;TZID=Europe/Rome:20180911T124500
DTSTAMP:20260510T145952
CREATED:20180725T064005Z
LAST-MODIFIED:20180725T064005Z
UID:4748-1536666300-1536669900@www.oa-roma.inaf.it
SUMMARY:The planet formation seen through high-resolution images of protoplanetary disks
DESCRIPTION:The high occurrence of exoplanets around solar-type stars suggests that planets form very efficiently in protoplanetary disks. Yet\, numerical simulations and laboratory experiments show that the planet formation is a complicated process. The onset of optical/NIR and (sub-)mm surveys of young stars has been a game changer for our understanding of protoplanetary disks and planet formation. Thanks to the contributed effort of VLT/SPHERE\, GPI\, and ALMA we could resolve with unprecedented resolution several sub-structures at the disk surface and midplane from few to hundreds of au from the star. I show the method and the recent improvement of this type of observations and discuss the implications to the recurrent existence of these disk features.
URL:https://www.oa-roma.inaf.it/event/colloquium-antonio-garufi-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20180911T114500
DTEND;TZID=Europe/Rome:20180911T124500
DTSTAMP:20260510T145952
CREATED:20180725T064005Z
LAST-MODIFIED:20180725T064005Z
UID:4154-1536666300-1536669900@www.oa-roma.inaf.it
SUMMARY:The planet formation seen through high-resolution images of protoplanetary disks
DESCRIPTION:The high occurrence of exoplanets around solar-type stars suggests that planets form very efficiently in protoplanetary disks. Yet\, numerical simulations and laboratory experiments show that the planet formation is a complicated process. The onset of optical/NIR and (sub-)mm surveys of young stars has been a game changer for our understanding of protoplanetary disks and planet formation. Thanks to the contributed effort of VLT/SPHERE\, GPI\, and ALMA we could resolve with unprecedented resolution several sub-structures at the disk surface and midplane from few to hundreds of au from the star. I show the method and the recent improvement of this type of observations and discuss the implications to the recurrent existence of these disk features.
URL:https://www.oa-roma.inaf.it/event/colloquium-antonio-garufi/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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