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Complex organic molecules tracing the comet-forming zones in protoplanetary disks

Published online by Cambridge University Press:  12 October 2020

Catherine Walsh
Affiliation:
School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK email: c.walsh1@leeds.ac.uk
John D. Ilee
Affiliation:
School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK email: c.walsh1@leeds.ac.uk
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Abstract

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Resolved emission from gas-phase methanol can reveal the abundance and distribution of the comet-forming ice reservoir in protoplanetary disks. ALMA Cycle 4 observations of four transitions of gas-phase methanol in TW Hya allow the first model-independent determination of the rotational temperature of methanol in a prototoplanetary disk. The data confirm that the methanol is rotationally cold (Trot < 50 K), and well constrain the column density to 2 × 1012 cm−2. Astrochemical models will constrain the chemical origin of methanol in TW Hya.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

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