Evolution of galaxy scaling relations in clusters at 0.5 < z < 1.5
Entity
UAM. Departamento de Física TeóricaPublisher
EDP SciencesDate
2021-02-01Citation
Astronomy & Astrophysics 646 (2021): A53ISSN
1432-0746; 0004-6361DOI
10.1051/0004-6361/201936456Editor's Version
https://doi.org/10.1051/0004-6361/201936456Subjects
Tully-Fisher Relation; Emission-Line Galaxies; Dominated Galaxies; Spectroscopic Survey Kross; Cl-1604 Supercluster; Dark-Matter Haloes; Angular-Momentum; Similar-To 1; Star-Formation; Spiral Galaxies; Galaxies: Evolution; Galaxies: Clusters: General; Galaxies: Kinematics and Dynamics; Galaxies: Clusters: Individual: Cl1604; FísicaRights
© ESO 2021
Files in this item
Google™ Scholar:Pérez-Martínez, J. M.
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Ziegler, B.
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Dannerbauer, H.
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Böhm, A.
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Verdugo, M.
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Díaz Beltrán, Ángeles Isabel
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Hoyos, C.
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