Boosting the evolutionary picture of Cl 0024+17 and MS 0451-03: A case study at intermediate-redshift

In this work we improve the dynamic-evolutionary framework of two massive clusters at intermediate redshifts: Cl 0024+17 at \(z \sim 0.4\) and MS 0451-03 at \(z \sim 0.5\). The spectroscopic galaxy members were selected from Moran et al. (2007a), which combine optical and UV imaging with spectroscop...

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Veröffentlicht in:	arXiv.org 2024-11
Hauptverfasser:	Costa, A P, Ribeiro, A L B, de Carvalho, R R, Benevides, J A
Format:	Artikel
Sprache:	eng
Schlagworte:	Cluster analysis Galactic clusters Galaxy distribution Kinematics Physics - Astrophysics of Galaxies Red shift Subgroups Velocity distribution
Online-Zugang:	Volltext
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