Journal article
PAHs as tracers of the molecular gas in star-forming galaxies
- Abstract:
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We combine new CO(1–0) line observations of 24 intermediate redshift galaxies (0.03 < z < 0.28) along with literature data of galaxies at 0 < z < 4 to explore scaling relations between the dust and gas content using polycyclic aromatic hydrocarbon (PAH) 6.2 μm (L6.2), CO (L′CO), and infrared (LIR) luminosities for a wide range of redshifts and physical environments. Our analysis confirms the existence of a universal L6.2–L′CO correlation followed by normal star-forming galaxies ...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 4.5MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/sty2777
Authors
Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 482
- Issue:
- 2
- Pages:
- 1618-1633
- Publication date:
- 2018-10-13
- Acceptance date:
- 2018-10-09
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Language:
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English
- Keywords:
- Pubs id:
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pubs:934905
- UUID:
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uuid:31dd2823-52e8-480b-b405-d6fd28ddf89a
- Local pid:
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pubs:934905
- Source identifiers:
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934905
- Deposit date:
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2019-02-21
Terms of use
- Copyright holder:
- Cortzen, I et al
- Copyright date:
- 2018
- Notes:
- Copyright © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
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