The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum
We study the baryonic Tully–Fisher relation (BTFR) at z ≃ 0 using 153 galaxies from the Spitzer Photometry and Accurate Rotation Curve sample. We consider different definitions of the characteristic velocity from H I and H α rotation curves, as well as H I line-widths from single-dish observations....
Huvudupphovsmän: | Lelli, F, McGaugh, S, Schombert, J, Desmond, H, Katz, H |
---|---|
Materialtyp: | Journal article |
Språk: | English |
Publicerad: |
Oxford University Press
2019
|
Liknande verk
Liknande verk
-
The Baryonic Tully–Fisher Relation. II. Stellar Mass Models
av: Francis Duey, et al.
Publicerad: (2025-01-01) -
The Baryonic Tully–Fisher Relation. I. WISE/Spitzer Photometry
av: Francis Duey, et al.
Publicerad: (2024-01-01) -
Indefinitely Flat Circular Velocities and the Baryonic Tully–Fisher Relation from Weak Lensing
av: Tobias Mistele, et al.
Publicerad: (2024-01-01) -
Stellar feedback and the energy budget of late-type Galaxies: Missing baryons and core creation
av: Katz, H, et al.
Publicerad: (2018) -
Uncorrelated velocity and size residuals across galaxy rotation curves
av: Desmond, H, et al.
Publicerad: (2019)