We use ALMA observations of CO(2–1) in 13 massive (
We explore how the presence of detectable molecular gas depends on the inferred star formation histories (SFHs) in eight massive, quiescent galaxies at
- NSF-PAR ID:
- 10380856
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 940
- Issue:
- 1
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 39
- Size(s):
- ["Article No. 39"]
- Sponsoring Org:
- National Science Foundation
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Abstract We measure the CO-to-H2conversion factor (
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