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arXiv · 1307.1687

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

Jean-François Gonzalez·Christophe Pinte·Sarah T. Maddison·François Ménard
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Abstract

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.

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Jean-François Gonzalez, Christophe Pinte, Sarah T. Maddison, François Ménard. 2013-07-05. Planet gaps in the dust layer of 3D proto-planetary disks: Observability with ALMA. https://doi.org/10.1017/s1743921313008053

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