Emergence of the Galaxy Morphology–Star Formation Activity–Clustercentric Radius Relations in Galaxy Clusters

We investigate when and how the relations of galaxy morphology and star-forming activity with clustercentric radius become evident in galaxy clusters. We identify 162 galaxy clusters with total mass Mtotcl>5×1013M⊙ at z = 0.625 in the Horizon Run 5 cosmological hydrodynamical simulation and study...

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Veröffentlicht in:	The Astrophysical Journal 2024-12, Vol.977 (2), p.183
Hauptverfasser:	Hong, Sungwook E., Park, Changbom, Mishra, Preetish K., Kim, Juhan, Gibson, Brad K., Kim, Yonghwi, Few, C. Gareth, Pichon, Christophe, Shin, Jihye, Lee, Jaehyun
Format:	Artikel
Sprache:	eng
Schlagworte:	Disks Galactic clusters Galaxies Galaxy clusters Galaxy distribution Galaxy evolution Galaxy interactions Mass distribution Morphology Sciences of the Universe Skewed distributions Spheroids Star & galaxy formation Star formation Star formation rate Stars Stars & galaxies Stellar mass
Online-Zugang:	Volltext
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