- Abstract:
-
We are just starting to understand the physical processes driving the dramatic change in cosmic star formation rate between z ∼ 2 and the present day. A quantity directly linked to star formation is the molecular gas density, which should be measured through independent methods to explore variations due to cosmic variance and systematic uncertainties. We use intervening CO absorption lines in the spectra of mm-bright background sources to provide a census of the molecular gas mass density of ...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Files:
-
- Publisher copy:
- 10.1093/mnras/stz2660
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 490
- Issue:
- 1
- Pages:
- 1220-1230
- Publication date:
- 2019-09-21
- Acceptance date:
- 2019-09-17
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Pubs id:
-
1075735
- Local pid:
- pubs:1075735
- Language:
- English
- Keywords:
- Copyright holder:
- Klitsch et al.
- Copyright date:
- 2019
- Rights statement:
- © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal article
ALMACAL – VI. Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
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