Zobrazeno 1 - 10
of 115
pro vyhledávání: '"Frazer R. Pearce"'
Autor:
Daniel J Cornwell, Ulrike Kuchner, Alfonso Aragón-Salamanca, Meghan E Gray, Frazer R Pearce, J Alfonso L Aguerri, Weiguang Cui, J Méndez-Abreu, Luis Peralta de Arriba, Scott C Trager
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 517, 1678-1694. Oxford University Press
Next-generation wide-field spectroscopic surveys will observe the infall regions around large numbers of galaxy clusters with high sampling rates for the first time. Here we assess the feasibility of extracting the large-scale cosmic web around clust
Autor:
Roan Haggar, Ulrike Kuchner, Meghan E Gray, Frazer R Pearce, Alexander Knebe, Gustavo Yepes, Weiguang Cui
Galaxy clusters grow by accreting galaxies as individual objects, or as members of a galaxy group. These groups can strongly impact galaxy evolution, stripping the gas from galaxies, and enhancing the rate of galaxy mergers. However, it is not clear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cb4139bd981d2d895c3395e09cd8247
http://arxiv.org/abs/2209.13604
http://arxiv.org/abs/2209.13604
Autor:
Weiguang Cui, Qingyang Li, E. Rasia, Romeel Davé, Marco De Petris, Frazer R. Pearce, Gustavo Yepes, John A. Peacock, Xiaohu Yang, Alexander Knebe
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Li, Q, Cui, W, Yang, X, Rasia, E, Dave, R, Petris, M D, Knebe, A, Peacock, J A, Pearce, F & Yepes, G 2020, ' The Three Hundred Project: the stellar and gas profiles ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2930-2948 . https://doi.org/10.1093/mnras/staa1385
Li, Q, Cui, W, Yang, X, Rasia, E, Dave, R, Petris, M D, Knebe, A, Peacock, J A, Pearce, F & Yepes, G 2020, ' The Three Hundred Project: the stellar and gas profiles ', Monthly Notices of the Royal Astronomical Society, vol. 495, no. 3, pp. 2930-2948 . https://doi.org/10.1093/mnras/staa1385
Using the catalogues of galaxy clusters from The Three Hundred project, modelled with both hydrodynamic simulations, (Gadget-X and Gadget-MUSIC), and semi-analytic models (SAMs), we study the scatter and self-similarity of the profiles and distributi
Autor:
Meghan E. Gray, U. Kuchner, Alfonso Aragón-Salamanca, Agustín Rost, Frazer R. Pearce, Gustavo Yepes, Weiguang Cui, Alexander Knebe, Roan Haggar
Publikováno v:
Kuchner, U, Haggar, R, Aragón-Salamanca, A, Pearce, F R, Gray, M E, Rost, A, Cui, W, Knebe, A & Yepes, G 2022, ' An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 510, no. 1, pp. 581-592 . https://doi.org/10.1093/mnras/stab3419
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Monthly Notices of the Royal Astronomical Society 510.1 (2022): 581
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::537b6ecb1d9704fca385d3a0242e1084
https://hdl.handle.net/20.500.11820/70cd866e-7c89-482a-8bd2-78161017b046
https://hdl.handle.net/20.500.11820/70cd866e-7c89-482a-8bd2-78161017b046
Autor:
Alfonso Aragón-Salamanca, Alexander Knebe, Agustín Rost, Ulrike Kuchner, Meghan E. Gray, Frazer R. Pearce, Elena Rasia, Gustavo Yepes, Weiguang Cui
Inferring line-of-sight distances from redshifts in and around galaxy clusters is complicated by peculiar velocities, a phenomenon known as the "Fingers of God" (FoG). This presents a significant challenge for finding filaments in large observational
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8106ba6a56cb08a12ce5db96f3aee844
https://doi.org/10.48550/arxiv.2102.12500
https://doi.org/10.48550/arxiv.2102.12500
Dark matter-only simulations are able to produce the cosmic structure of a $\Lambda$CDM universe, at a much lower computational cost than more physically motivated hydrodynamical simulations. However, it is not clear how well smaller substructure is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c03cbb886cb28d3e2102b0828dc2e76
https://doi.org/10.48550/arxiv.2101.03178
https://doi.org/10.48550/arxiv.2101.03178
Autor:
Claudia del P. Lagos, Robert Mostoghiu, Chris Power, Frazer R. Pearce, Alexander Knebe, Klaus Dolag, Gustavo Yepes, Giuseppe Murante, Weiguang Cui, Stefano Borgani
Using 324 numerically modelled galaxy clusters as provided by THE THREE HUNDRED project, we study the evolution of the kinematic properties of the stellar component of haloes on first infall. We select objects with M$_{\textrm{star}}>5\times10^{10} h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53a1bbd4957450973104cfe63f86e455
Autor:
Alexander Knebe, Meghan E. Gray, Roan Haggar, Frazer R. Pearce, Weiguang Cui, Gustavo Yepes, Robert Mostoghiu
Publikováno v:
Monthly Notices of the Royal Astronomical Society
In the outer regions of a galaxy cluster, galaxies may be either falling into the cluster for the first time, or have already passed through the cluster centre at some point in their past. To investigate these two distinct populations, we utilise The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9aa1b944b2d5e25be066e4377d8910a7
Autor:
E. Puchwein, Daniel Cunnama, Scott T. Kay, Pascal J. Elahi, Alexander Knebe, Frazer R. Pearce, Stefano Borgani, Charlotte Welker, Romeel Davé, Chris Power, Joop Schaye, Gustavo Yepes, Ian G. McCarthy, Weiguang Cui
Publikováno v:
Power, C, Elahi, P J, Welker, C, Knebe, A, Pearce, F R, Yepes, G, Dave, R, Kay, S T, McCarthy, I G, Puchwein, E, Borgani, S, Cunnama, D, Cui, W & Schaye, J 2020, ' nIFTy Galaxy Cluster simulations VI. The dynamical imprint of substructure on gaseous cluster outskirts ', Monthly Notices of the Royal Astronomical Society, vol. 491, no. 3, pp. 3923-3936 . https://doi.org/10.1093/mnras/stz3176
Monthly Notices of the RAS (0035-8711), 491(3), 3923-3936
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the RAS (0035-8711), 491(3), 3923-3936
Monthly Notices of the Royal Astronomical Society
Galaxy cluster outskirts mark the transition region from the mildly non-linear cosmic web to the highly non-linear, virialised, cluster interior. It is in this transition region that the intra-cluster medium (ICM) begins to influence the properties o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::158e5478fd37b9ada737d3566ae3f6fc
https://hdl.handle.net/1887/3141964
https://hdl.handle.net/1887/3141964
Autor:
Marco De Petris, Chris Power, Matías Gámez-Marín, Alexander Knebe, Roan Haggar, Kai Hoffmann, Weiguang Cui, Frazer R. Pearce, Robert Mostoghiu
Using 324 numerically modelled galaxy clusters we investigate the radial and galaxy-halo alignment of dark matter subhaloes and satellite galaxies orbiting within and around them. We find that radial alignment depends on distance to the centre of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f52c3f57e67bb18a53b6899a35ac1e5
http://hdl.handle.net/11573/1417899
http://hdl.handle.net/11573/1417899