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...
Egile Nagusiak: | Topal, S, Bureau, M, Tiley, A, Davis, T, Torii, K |
---|---|
Formatua: | Journal article |
Argitaratua: |
Oxford University Press
2018
|
Antzeko izenburuak
-
The Tully–Fisher relation of COLD GASS galaxies
nork: Tiley, A, et al.
Argitaratua: (2016) -
The Tully-Fisher relation of COLD GASS galaxies
nork: Bureau, M, et al.
Argitaratua: (2016) -
The Tully-Fisher relations of early-type spiral and S0 galaxies
nork: Williams, M, et al.
Argitaratua: (2010) -
A Shared Tully-Fisher Relation for Spirals and S0 Galaxies
nork: Williams, M, et al.
Argitaratua: (2009) -
Dark Matter and the Tully-Fisher Relations of Spiral and S0 Galaxies
nork: Williams, M, et al.
Argitaratua: (2010)