The Radial Acceleration Relation in CLASH Galaxy Clusters

The radial acceleration relation (RAR) in galaxies describes a tight empirical scaling law between the total acceleration observed in galaxies and that expected from their baryonic mass , with a characteristic acceleration scale of m s−2. Here, we examine if such a correlation exists in galaxy clust...

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Veröffentlicht in:	The Astrophysical journal 2020-06, Vol.896 (1), p.70
Hauptverfasser:	Tian, Yong, Umetsu, Keiichi, Ko, Chung-Ming, Donahue, Megan, Chiu, I-Non
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Baryons Cosmology Dark matter Galactic clusters Galaxies Galaxy clusters Gravitational lensing Intracluster medium Scaling laws Stars & galaxies Stellar mass Supernova X-ray astronomy
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