CO Tully–Fisher relation of star-forming galaxies at = 0.05–0.3
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 ga...
| Päätekijät: | , , , , |
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| Aineistotyyppi: | Journal article |
| Julkaistu: |
Oxford University Press
2018
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