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The Structure and Evolution of Protoplanetary Disks: an Infrared and Submillimeter View

Published online by Cambridge University Press:  27 January 2016

Lucas A. Cieza
Lucas A. Cieza*
Affiliation:
Núcleo de Astronomía, Universidad Diego Portales, Chile email: lucas.cieza@mail.udp.cl
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Abstract

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Circumstellar disks are the sites of planet formation, and the very high incidence of extrasolar planets implies that most of them actually form planetary systems. Studying the structure and evolution of protoplanetary disks can thus place important constraints on the conditions, timescales, and mechanisms associated with the planet formation process. In this review, we discuss observational results from infrared and submillimeter wavelength studies. We review disk lifetimes, transition objects, disk demographics, and highlight a few remarkable results from ALMA Early Science observations. We finish with a brief discussion of ALMA's potential to transform the field in near future.

Keywords

protoplanetary disksinfrared: planetary systemssubmillimeter: planetary systems
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 128 - 134
Copyright
Copyright © International Astronomical Union 2016 

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