Constraints on the Physical Origin of Large Cavities in Transition Disks from Multiwavelength Dust Continuum Emission

The physical origin of the large cavities observed in transition disks is to date still unclear. Different physical mechanisms (e.g., a companion, dead zones, enhanced grain growth) produce disk cavities of different depth, and the expected spatial distribution of gas and solids in each mechanism is...

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Xehetasun bibliografikoak

Egile Nagusiak:	Anibal Sierra, Laura M. Pérez, Benjamín Sotomayor, Myriam Benisty, Claire J. Chandler, Sean Andrews, John Carpenter, Thomas Henning, Leonardo Testi, Luca Ricci, David Wilner
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2024-01-01
Saila:	The Astrophysical Journal
Gaiak:	Protoplanetary disks Circumstellar dust Millimeter astronomy Submillimeter astronomy Radio interferometry
Sarrera elektronikoa:	https://doi.org/10.3847/1538-4357/ad7460
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