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Spiral density waves in a young protoplanetary disk

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Gravitational forces are expected to excite spiral density waves in protoplanetary disks, disks of gas and dust orbiting young stars. However, previous observations that showed spiral structure were not able to probe disk midplanes, where most of the mass is concentrated and where planet formation t...

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Bibliographic Details
Main Authors: Pérez, Laura M. (Author) , Dullemond, Cornelis (Author)
Format: Article (Journal)
Language:English
Published: 2016
In: Science
Year: 2016, Volume: 353, Issue: 6307, Pages: 1519-1521
ISSN:1095-9203
DOI:10.1126/science.aaf8296
Online Access:Verlag, Volltext: http://dx.doi.org/10.1126/science.aaf8296
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Author Notes:Laura M. Pérez, John M. Carpenter, Sean M. Andrews, Luca Ricci, Andrea Isella, Hendrik Linz, Anneila I. Sargent, David J. Wilner, Thomas Henning, Adam T. Deller, Claire J. Chandler, Cornelis P. Dullemond, Joseph Lazio, Karl M. Menten, Stuartt A. Corder, Shaye Storm, Leonardo Testi, Marco Tazzari, Woojin Kwon, Nuria Calvet, Jane S. Greaves, Robert J. Harris, Lee G. Mundy

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