Chemical Modeling of Orion Nebula Cluster Disks: Evidence for Massive, Compact Gas Disks with Interstellar Gas-to-dust Ratios
The stellar cluster environment is expected to play a central role in the evolution of circumstellar disks. We use thermochemical modeling to constrain the dust and gas masses, disk sizes, UV and X-ray radiation fields, viewing geometries, and central stellar masses of 20 class II disks in the Orion...
Main Authors: | Ryan D. Boyden, Josh A. Eisner |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acaf77 |
Similar Items
-
The –M disk Relationship for Herbig Ae/Be Stars: A Lifetime Problem for Disks with Low Masses?
by: Sierra L. Grant, et al.
Published: (2023-01-01) -
Ring Gap Structure around Class I Protostar WL 17
by: Ayumu Shoshi, et al.
Published: (2024-01-01) -
Coagulation–Fragmentation Equilibrium for Charged Dust: Abundance of Submicron Grains Increases Dramatically in Protoplanetary Disks
by: Vitaly Akimkin, et al.
Published: (2023-01-01) -
Spectroastrometric Survey of Protoplanetary Disks with Inner Dust Cavities
by: Stanley K. Jensen Jr., et al.
Published: (2024-01-01) -
Sites of Planet Formation in Binary Systems. I. Evidence for Disk−Orbit Alignment in the Close Binary FO Tau
by: Benjamin M. Tofflemire, et al.
Published: (2024-01-01)