The SAMI galaxy survey: Mass and environment as independent drivers of galaxy dynamics

ABSTRACT The kinematic morphology–density relation of galaxies is normally attributed to a changing distribution of galaxy stellar masses with the local environment. However, earlier studies were largely focused on slow rotators; the dynamical properties of the overall population in relation to envi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2021-12, Vol.508 (2), p.2307-2328
Hauptverfasser:	van de Sande, Jesse, Croom, Scott M, Bland-Hawthorn, Joss, Cortese, Luca, Scott, Nicholas, Lagos, Claudia D P, D’Eugenio, Francesco, Bryant, Julia J, Brough, Sarah, Catinella, Barbara, Foster, Caroline, Groves, Brent, Harborne, Katherine E, López-Sánchez, Ángel R, McDermid, Richard, Medling, Anne, Owers, Matt S, Richards, Samuel N, Sweet, Sarah M, Vaughan, Sam P
Format:	Artikel
Sprache:	eng
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