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...

Volledige beschrijving

Bibliografische gegevens

Hoofdauteurs:	Anibal Sierra, Laura M. Pérez, Benjamín Sotomayor, Myriam Benisty, Claire J. Chandler, Sean Andrews, John Carpenter, Thomas Henning, Leonardo Testi, Luca Ricci, David Wilner
Formaat:	Artigo
Taal:	Inglês
Gepubliceerd in:	IOP Publishing 2024-01-01
Reeks:	The Astrophysical Journal
Onderwerpen:	Protoplanetary disks Circumstellar dust Millimeter astronomy Submillimeter astronomy Radio interferometry
Online toegang:	https://doi.org/10.3847/1538-4357/ad7460
Tags:	Voeg label toe Geen labels, Wees de eerste die dit record labelt!