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SUMMARY:A Dusty Origin for the Correlation Between Protoplanetary Disc Acc
 retion Rates and Dust Masses - Andrew Sellek
DTSTART:20210120T133000Z
DTEND:20210120T140000Z
UID:TALK155845@talks.cam.ac.uk
CONTACT:Emma Curtis Lake
DESCRIPTION:I will talk about how trends observed in demographic studies o
 f protoplanetary discs enable us to test our models of the various process
 es that deplete and disperse the disc material. In particular I will show 
 how applying dust evolution models to recent data on accretion rates and m
 asses in the Lupus and Upper Scorpius star forming regions helps resolve t
 ensions in the data and places valuable constraints on both turbulence and
  photoevaporation.
LOCATION: Webinar  (via Zoom online)
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