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Radio Interferometry Observations of the Hallmarks of Planet Formation

Published online by Cambridge University Press:  06 January 2014

Sean M. Andrews
Sean M. Andrews*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, Massachusetts 02138, USA email: sandrews@cfa.harvard.edu
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Abstract

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Some of the fundamental processes involved in the evolution of circumstellar disks and the assembly of planetary systems are just now becoming accessible to astronomical observations. The new promise of observational work in the field of planet formation makes for a very dynamic research scenario, which is certain to be amplified in the coming years as the revolutionary Atacama Large Millimeter/submillimeter Array (ALMA) facility ramps up to full operations. To highlight the new directions being explored in these fields, this brief review will describe how high angular resolution measurements at millimeter/radio wavelengths are being used to study several crucial aspects of the formation and early evolution of planetary systems, including: the gas and dust structures of protoplanetary disks, the growth and migration of disk solids, and the interactions between a young planetary system and its natal, gas-rich disk.

Keywords

circumstellar matterplanetary systems: formationplanetary systems: protoplanetary disksradio continuum: starsradio lines: starssubmillimeter
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. 80 - 89
Copyright
Copyright © International Astronomical Union 2013 

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