BEGIN:VCALENDAR
VERSION:2.0
PRODID:https://murmitoyen.com/events/vanille/udem/
X-WR-TIMEZONE:America/Montreal
BEGIN:VEVENT
UID:69dac27d9b11c
DTSTAMP:20260411T175157
DTSTART:20180307T103000
SEQUENCE:0
TRANSP:OPAQUE
DTEND:20180307T103000
URL:https://murmitoyen.com/events/vanille/udem/detail/810846-from-cosmic-du
 st-to-planetesimals-models-vs-observations
LOCATION:Université de Montréal - Pavillon Claire-McNicoll\, 2900\, chemi
 n de la Tour\, Montréal\, QC\, Canada\, H3T 1J6
SUMMARY:From Cosmic Dust to Planetesimals: Models vs. Observations
DESCRIPTION:Conférence de  Paola Pinilla (Arizona).
\nRésumé :In this n
 ew era of powerful telescopes such as the Atacama Large Millimeter/submill
 imeter Array\, we are now able to study the birth of planets in disks arou
 nd young stars\, in more detail than ever before.  These new observations
  are revealing fascinating structures in protoplanetary disks that are tra
 nsforming our understanding of the formation and evolution of planetary sy
 stems. In this talk\, I will explain theoretical models of dust evolution 
 in protoplanetary disks\, in particular the dynamics and growth from cosmi
 c dust to planetesimals. I will compare these theoretical predictions with
  current multi-wavelength observations of protoplanetary disks. This link 
 is providing significant insights about how different physical conditions 
 play a crucial role in the formation of planetesimals\, and is extending o
 ur understanding of how initial conditions of protoplanetary disks are ref
 lected in the large diversity of extrasolar systems.  I will finish with
  future perspectives in the field\, in particular about expanding our unde
 rstanding of planet formation in physically diverse environments.
END:VEVENT
BEGIN:VTIMEZONE
TZID:America/Montreal
X-LIC-LOCATION:America/Montreal
END:VTIMEZONE
END:VCALENDAR