Área de investigación | Astronomía, Espacio y Ciencias de la Tierra |
Título | THE THREE HUNDRED project: the gas disruption of infalling objects in cluster environments |
Tipo de publicación | Artículo de revista |
Año de publicación | 2021 |
Autores | Mostoghiu, R, Arthur, J, Pearce, FR, Gray, M, Knebe, A, Cui, W, Welker, C, Cora, SA, Murante, G, Dolag, K, Yepes, G |
Revista | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
Volumen | 501 |
Número | 4 |
Páginas | 5029-5041 |
Type of Article | Article |
Palabras claves | galaxies: evolution, galaxies: interactions, methods: numerical |
Abstract | We analyse the gas content evolution of infalling haloes in cluster environments from The Three Hundred project, a collection of 324 numerically modelled galaxy clusters. The haloes in our sample were selected within 5R(200) of the main cluster halo at = 0 and have total halo mass M-200 >= 10(11)h(-1)M(circle dot). We track their main progenitors and study their gas evolution since their crossing into the infall region, which we define as 1-4R(200). Studying the radial trends of our populations using both the full phase-space information and a line-of-sight projection, we confirm the Arthur et al. (2019) result and identify a characteristic radius around 1.7R(200) in 3D and at R-200 in projection at which infalling haloes lose nearly all of the gas prior their infall. Splitting the trends by subhalo status,we show that subhaloes residing in group-mass and low-mass host haloes in the infall region follow similar radial gas-loss trends as their hosts, whereas subhaloes of cluster-mass host haloes are stripped of their gas much further out. Our results show that infalling objects suffer significant gaseous disruption that correlates with time-since-infall, cluster-centric distance, and host mass, and that the gaseous disruption they experience is a combination of subhalo pre-processing and object gas depletion at a radius that behaves like an accretion shock. |
DOI | 10.1093/mnras/stab014 |