Deep Search for Molecular Oxygen in TW Hya
The dominant form of oxygen in cold molecular clouds is gas-phase carbon monoxide (CO) and ice-phase water (H _2 O). Yet, in planet-forming disks around young stars, gas-phase CO and H _2 O are less abundant relative to their interstellar medium values, and no other major oxygen-carrying molecules h...
Main Authors: | Becky J. Williams, L. Ilsedore Cleeves, Christian Eistrup, Jon P. Ramsey |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acf717 |
Similar Items
-
The Surprising Evolution of the Shadow on the TW Hya Disk
by: John Debes, et al.
Published: (2023-01-01) -
A Census of the TW Hya Association with Gaia
by: K. L. Luhman
Published: (2023-01-01) -
How Large Is a Disk—What Do Protoplanetary Disk Gas Sizes Really Mean?
by: Leon Trapman, et al.
Published: (2023-01-01) -
Chemistry of Complex Organic Molecules in the V883 Ori Disk Revealed by ALMA Band 3 Observations
by: Yoshihide Yamato, et al.
Published: (2024-01-01) -
Disentangling CO Chemistry in a Protoplanetary Disk Using Explanatory Machine-learning Techniques
by: Amina Diop, et al.
Published: (2024-01-01)