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Zooming in on the Chemistry of Protoplanetary Disks with ALMA

Published online by Cambridge University Press:  04 September 2018

L. Ilsedore Cleeves Open the ORCID record for L. Ilsedore Cleeves [Opens in a new window]
L. Ilsedore Cleeves*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St MS-51, Cambridge, MA 02138, USA email: ilse.cleeves@cfa.harvard.edu
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Abstract

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During the first few ~Myr of a young stars life, it is encircled by a disk made up of molecular gas, dust, and ice – the building blocks for future planetary systems. How/when these disks form planets and what sets the planets initial compositions remain key outstanding questions in disk science. In recent years, major leaps in sensitivity and spatial resolution afforded by the Atacama Large Millimeter/Submillimeter Array (ALMA) have revolutionized our understanding of protoplanetary disks chemical composition and physical properties, revealing in some cases complex radial, vertical, and azimuthal structure in the dust and gas. In this contribution, I review recent observational results and new theoretical puzzles, and how these fit into a newly emerging picture of the disk environment.

Keywords

planetary systems: protoplanetary disksastrochemistry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S332: Astrochemistry VII: Through the Cosmos from Galaxies to Planets , March 2017 , pp. 57 - 68
Copyright
Copyright © International Astronomical Union 2018 

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