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Planet gaps in the dust layer of 3D proto-planetary disks: Observability with ALMA

Published online by Cambridge University Press:  06 January 2014

J.-F. Gonzalez ,
C. Pinte ,
S. T. Maddison  and
F. Ménard
J.-F. Gonzalez
Affiliation:
Université de Lyon, Lyon, F-69003, France; Université Lyon 1, Observatoire de Lyon, 9 avenue Charles André, Saint-Genis Laval, F-69230, France; CNRS, UMR 5574, Centre de Recherche Astrophysique de Lyon; École Normale Supérieure de Lyon, Lyon, F-69007, France email: Jean-Francois.Gonzalez@ens-lyon.fr
C. Pinte
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble, UMR 5274, Grenoble, F-38041, France email: christophe.pinte@obs.ujf-grenoble.fr, francois.menard@obs.ujf-grenoble.fr
S. T. Maddison
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia email: smaddison@swin.edu.au
F. Ménard
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble, UMR 5274, Grenoble, F-38041, France email: christophe.pinte@obs.ujf-grenoble.fr, francois.menard@obs.ujf-grenoble.fr
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Abstract

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Among the numerous known extrasolar planets, only a handful have been imaged directly so far, at large orbital radii and in rather evolved systems. The Atacama Large Millimeter/submillimeter Array (ALMA) will have the capacity to observe these wide planetary systems at a younger age, thus bringing a better understanding of the planet formation process. Here we explore the ability of ALMA to detect the gaps carved by planets on wide orbits.

Keywords

Planetary systems: protoplanetary disksradiative transfermethods: numericalsubmillimeter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 115 - 116
Copyright
Copyright © International Astronomical Union 2013 

References

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Pinte, C., Ménard, F., Duchêne, G., & Bastien, P. 2006, A&A, 459, 797Google Scholar
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