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14:00
If you have a question about this talk, please contact Emma Curtis Lake.
I will talk about how trends observed in demographic studies of protoplanetary discs enable us to test our models of the various processes that deplete and disperse the disc material. In particular I will show how applying dust evolution models to recent data on accretion rates and masses in the Lupus and Upper Scorpius star forming regions helps resolve tensions in the data and places valuable constraints on both turbulence and photoevaporation.
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Andrew Sellek , Institute Of Astronomy Seminars , Astronomy Seminars , Dusty Origin , Emma Curtis , Upper Scorpius , University Of Cambridge , நிறுவனம் ஆஃப் வானியல் கருத்தரங்குகள் , வானியல் கருத்தரங்குகள் , தூசி நிறைந்த ஆரிஜிந் , எம்மா கர்டிஸ் , பல்கலைக்கழகம் ஆஃப் கேம்பிரிட்ஜ் ,