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CO Tully–Fisher relation of star-forming galaxies at = 0.05–0.3

Abstract:

The Tully–Fisher relation (TFR) is an empirical relation between galaxy luminosity and rotation velocity. We present here the first TFR of galaxies beyond the local Universe that uses carbon monoxide (CO) as the kinematic tracer. Our final sample includes 25 isolated, non-interacting star-forming galaxies with double-horned or boxy CO integrated line profiles located at redshifts z ≤ 0.3, drawn from a larger ensemble of 67 detected objects. The best reverse Ks-band, stellar mass and baryonic ...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/sty1617

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Institution:
University of Oxford
Department:
Physics
Oxford college:
Wadham College
ORCID:
0000-0003-4980-1012
More by this author
ORCID:
0000-0003-4932-9379
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
479
Issue:
3
Pages:
3319–3334
Publication date:
2018-06-19
Acceptance date:
2018-06-15
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:890153
URN:
uri:070e1a3e-81a0-4fd9-8ee8-e9d18b091e39
UUID:
uuid:070e1a3e-81a0-4fd9-8ee8-e9d18b091e39
Local pid:
pubs:890153

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