Uncorrelated velocity and size residuals across galaxy rotation curves

The mass–velocity–size relation of late-type galaxies decouples into independent correlations between mass and velocity (the Tully–Fisher relation), and between mass and size. This behaviour is different to early-type galaxies which lie on a Fundamental Plane. We study the coupling of the Tully–Fish...

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Detalles Bibliográficos
Autores principales: Desmond, H, Katz, H, Lelli, F, McGaugh, S
Formato: Journal article
Lenguaje:English
Publicado: Oxford University Press 2019