BEGIN:VCALENDAR
VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260521T173021Z
UID:https://www.mpia.de/events/33065/5277135
DTSTART;VALUE=DATE:20221213
DTEND;VALUE=DATE:20221217
CLASS:PUBLIC
CREATED:20221205T092119Z
DESCRIPTION:Given the immense amount of information that can be gained from
  cloud-scale (~100pc) resolution multi-wavelength datasets on nearby galax
 ies like those provided by the PHANGS (Physics at High Angular resolution 
 in Nearby GalaxieS) survey and well as the tremendous progress made in sim
 ulating the star formation process in nearby galaxies at pc resolution\, i
 t seems timely to bring together experts from both the theoretical and obs
 ervational side to discuss how to answer pressing open question related to
  the physics of the star formation process (including interstellar medium 
 (ISM)).
LAST-MODIFIED:20221205T093205Z
LOCATION:International Academic Forum Heidelberg
SUMMARY:Theory meets Observations
URL;VALUE=URI:https://www.mpia.de/events/33065/5277135
END:VEVENT
END:VCALENDAR