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A `Rosetta Stone' for Protoplanetary Disks: The Synergy of Multi-Wavelength Observations

Abstract : Recent progress in telescope development has brought us different ways to observe protoplanetary disks: interferometers, space missions, adaptive optics, polarimetry, and time- and spectrally-resolved data. While the new facilities have changed the way we can tackle open problems in disk structure and evolution, there is a substantial lack of interconnection between different observing communities. Here, we explore the complementarity of some of the state-of-the-art observing techniques, and how they can be brought together to understand disk dispersal and planet formation.
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Contributor : Nathalie POTHIER Connect in order to contact the contributor
Submitted on : Monday, May 16, 2022 - 3:44:44 PM
Last modification on : Monday, July 4, 2022 - 9:44:43 AM

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A. Sicilia-Aguilar, A. Banzatti, A. Carmona, T. Stolker, M. Kama, et al.. A `Rosetta Stone' for Protoplanetary Disks: The Synergy of Multi-Wavelength Observations. Publications of the Astronomical Society of Australia, 2016, 33, ⟨10.1017/pasa.2016.56⟩. ⟨insu-03669393⟩



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