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| DOI | 10.1017/PASA.2016.7 | ||||
| Año | 2016 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Resolved observations are bringing new constraints on the origin of radial gaps in protoplanetary disks. The kinematics, sampled in detail in one case-study, are indicative of non-Keplerian flows, corresponding to warped structures and accretion which may both play a role in the development of cavities. Disk asymmetries seen in the radio continuum are being interpreted in the context of dust segregation via aerodynamic trapping. We summarise recent observational progress, and describe prospects for improvements in the near term.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | CASASSUS-MONTERO, SIMON PABLO | Hombre |
Universidad de Chile - Chile
Nucleo Milenio Discos Protoplanetarios - Chile |
| Agradecimiento |
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| We thank the following disk workers for very useful input: Henning Avenhaus, Amelia Bayo, Mark Booth, Valentin Christiaens, Lucas Cieza, Sebastian Marino, Matias Montesinos, Johan Olofsson, Sebastian Perez, Dave Principe, Nienke van der Marel, Gerrit van der Plas and Matthias Schreiber. Financial support was provided by Millennium Nucleus RC130007 (Chilean Ministry of Economy), and additionally by FONDECYT grant 1130949. |