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SUMMARY:A cloud-scale view on molecular gas and star formation in nearby g
 alaxies - Eva Schinnerer(MPIA)
DTSTART:20260129T160000Z
DTEND:20260129T170000Z
UID:TALK242032@talks.cam.ac.uk
CONTACT:133030
DESCRIPTION:Star formation is a vital process for stellar mass growth duri
 ng the evolution of galaxies. Our understanding of where stars form and ho
 w their formation is regulated across galactic disks is surprisingly incom
 plete. Cloud-scale observations that resolve the sites of recent (or futur
 e) star formation and allow for sampling the time evolution of the star fo
 rmation process have become possible with instruments such as ALMA\, HST\,
  VLT/MUSE and recently JWST.\nComprehensive surveys such as PHANGS (Physic
 s at High Angular resolution in Nearby GalaxieS) enabling the study of the
  molecular gas reservoir\, dust and embedded star formation\, young stella
 r clusters and stellar feedback at comparable resolution have provided fir
 st robust insights on how \nthe molecular gas—star formation—stellar f
 eedback cycle depends on environment.
LOCATION:Hoyle Lecture Theatre\, Institute of Astronomy (and online - deta
 ils to be sent by e-mail)
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