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SUMMARY:A Post-Processing Pipeline for Proto-Planetary Disk Simulations (P
 PPPPDS)
DTSTART;VALUE=DATE-TIME:20200513T133000Z
DTEND;VALUE=DATE-TIME:20200513T135000Z
DTSTAMP;VALUE=DATE-TIME:20241101T160808Z
UID:indico-contribution-13@meetings.aip.de
DESCRIPTION:Speakers: Jon Ramsey (Virginia Initiative on Cosmic Origins\, 
 Department of Astronomy\, University of Virginia)\nI will present a new po
 st-processing pipeline for (magneto-)hydrodynamic simulations of protoplan
 etary accretion disks and results from its first application. By combining
  publicly available radiative transfer and astrochemistry tools\, we proce
 ss snapshots from radiative\, non-ideal MHD simulations of thermally-assis
 ted centrifugal outflows from disks (Gressel et al. 2020) to search for ob
 servational signposts of outflows which are accessible from current observ
 atories. In particular\, we compare synthetic observations from models wit
 h and without outflows to determine which transitions and chemical species
  can be used to distinguish between the two classes of models. We find tha
 t the shape of the line profiles\, and velocity asymmetries in moment 1 ma
 ps\, can discriminate between disks with and without outflows. By combinin
 g the synthetic observations with the full simulation data\, we can also p
 inpoint where emission from a particular line or species is coming from in
  the outflow and/or disk\, which can help us better understand existing an
 d future observations of disks and outflows.\n\nhttps://iaus379.aip.de/eve
 nt/1/contributions/13/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://iaus379.aip.de/event/1/contributions/13/
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