The Arizona Molecular ISM Survey with the SMT: Variations in the CO(2–1)/CO(1–0) Line Ratio across the Galaxy Population
The J = 1 → 0 spectral line of carbon monoxide (CO(1–0)) is the canonical tracer of molecular gas. However, CO(2–1) is frequently used in its place, following the assumption that the higher-energy line can be used to infer the CO(1–0) luminosity and molecular gas mass. The use of CO(2–1) depends on...
Saved in:
| Main Authors: | Ryan P. Keenan, Daniel P. Marrone, Garrett K. Keating |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ada361 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
A Comparative Study of the Ground State Transitions of CO and C i as Molecular Gas Tracers at High Redshift
by: Marta Frias Castillo, et al.
Published: (2025-01-01) -
Pushing the Atacama Large Millimeter/submillimeter Array to the Limit: 140 pc Resolution Observations of a z = 6.6 Quasar–Galaxy Merger Resolve Strikingly Different Morphologies of Dust Continuum and [C ii] 158 μm Emission
by: Romain A. Meyer, et al.
Published: (2025-01-01) -
PHIBSS: Searching for Molecular Gas Outflows in Star-forming Galaxies at z = 0.5–2.6
by: Capucine Barfety, et al.
Published: (2025-01-01) -
Application of Resolved Low-J Multi-CO Line Modeling with RADEX to Constrain the Molecular Gas Properties in the Starburst M82
by: Valencia Zhang, et al.
Published: (2025-01-01) -
The SUPERCOLD-CGM Survey. II. [C i](1–0) Emission and the Physical Conditions of Cold Gas in Enormous Lyα Nebulae at z ∼ 2
by: Jianan Li, et al.
Published: (2024-01-01)