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SUMMARY:ALMA chemical survey of Disk-Outflow sources in Taurus
DTSTART;VALUE=DATE-TIME:20200512T145000Z
DTEND;VALUE=DATE-TIME:20200512T151000Z
DTSTAMP;VALUE=DATE-TIME:20240704T115618Z
UID:indico-contribution-18@meetings.aip.de
DESCRIPTION:Speakers: Antonio Garufi ()\nALMA-DOT is a small campaign devo
 ted to the chemical characterization of disk-outflow sources in Taurus. Th
 e sample currently consists of six Class I sources known to drive powerful
  outflows. The high angular resolution and sensitivity of ALMA allowed us 
 to characterize their chemical composition by separating the disk emission
  from the outflow and envelope contamination. Six molecules - from carbon 
 monoxyde to the simple organic formaldehyde and methanol - have been surve
 yed in each target. I present the results of the survey\, shedding light o
 n (i) the timescale for the formation of dust and gas sub-structures\, (ii
 ) the morphological interplay of dust and gas\, (iii) the role of disk-fee
 ding filaments\, (iv) the distribution and formation mechanism of simple o
 rganic molecules\, and (v) the chemical composition of molecular outflows.
  Young sources like those probed by ALMA-DOT offer the best laboratory to 
 study how soon are planets formed and how are complex molecules delivered 
 to the (assembling) planetary atmospheres.\n\nhttps://meetings.aip.de/even
 t/1/contributions/18/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/1/contributions/18/
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