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Observation of Chemistry in Protoplanetary Disks

Published online by Cambridge University Press:  23 September 2016

Anne Dutrey
Anne Dutrey*
Affiliation:
Observatoire de Bordeaux, 2 rue de l'observatoire, F-33270 Floirac, France

Abstract

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Protoplanetary disks are now intensively observed by mm arrays. While resolved images of CO rotation lines permit a better understanding of their physical structure, molecular surveys provided by current mm telescopes are currently sensitivity limited and do not allow a quantitative analysis of the chemical properties of disks. In this paper, I review the actual observational knowledge of the chemistry in the outer disks surrounding low and intermediate PMS stars and traced by mm data.

Type
Part 8: Disks
Information
Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 411 - 416
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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