Zobrazeno 1 - 10
of 65
pro vyhledávání: '"C Ragone-Figueroa"'
Autor:
Veronica Biffi, Vicent Quilis, Stefano Borgani, E. Rasia, Gian Luigi Granato, Klaus Dolag, Susana Planelles, Giuseppe Murante, C. Ragone-Figueroa
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:5703-5719
Cosmological shock waves are ubiquitous to cosmic structure formation and evolution. As a consequence, they play a major role in the energy distribution and thermalization of the intergalactic medium (IGM). We analyze the Mach number distribution in
Autor:
Roberto De Propris, Diego G. Lambas, Elena A. Romashkova, Michael J. West, C. Ragone-Figueroa, Kishore C. Patra, Felipe Andrade-Santos, E. Rasia, Christine Jones, William R. Forman, Stefano Borgani, Rain Kipper
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We explore the persistence of the alignment of brightest cluster galaxies (BCGs) with their local environment. We find that a significant fraction of BCGs do not coincide with the centroid of the X-ray gas distribution and/or show peculiar velocities
Nowadays, Machine Learning techniques offer fast and efficient solutions for classification problems that would require intensive computational resources via traditional methods. We examine the use of a supervised Random Forest to classify stars in s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d86dede1e27f4d93b2909635eea642c4
https://hdl.handle.net/11368/3029739
https://hdl.handle.net/11368/3029739
Akademický článek
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Autor:
I. Marini, C. Ragone-Figueroa, Giuseppe Murante, A. Saro, Barbara Sartoris, A Ragagnin, Gian Luigi Granato, Klaus Dolag, Stefano Borgani, Yang Wang
Using the DIANOGA hydrodynamical zoom-in simulation set of galaxy clusters, we analyze the dynamics traced by stars belonging to the Brightest Cluster Galaxies (BCGs) and their surrounding diffuse component, forming the intracluster light (ICL), and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68fd24c4a3d486a33f1c1cad1c19fd0c
http://hdl.handle.net/11368/3029738
http://hdl.handle.net/11368/3029738
Autor:
Nicola R. Napolitano, W. Lin, Giuliano Taffoni, Gian Luigi Granato, L. Tornatore, E. Rasia, C. Ragone-Figueroa, L. Bassini, A. Ragagnin, Klaus Dolag, Yang Wang, Giuseppe Murante, V. Biffi, Stefano Borgani
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We studied the star formation rate (SFR) in cosmological hydrodynamical simulations of galaxy (proto-)clusters in the redshift range $0
Comment: 20 pages, 19 figures. Accepted for publication in A&A
Comment: 20 pages, 19 figures. Accepted for publication in A&A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ac89c07296eca5611a310d8ec5573dd
http://hdl.handle.net/11368/2991710
http://hdl.handle.net/11368/2991710
Autor:
E. Rasia, R. De Propris, D García Lambas, Stefano Borgani, C. Ragone-Figueroa, Giuseppe Murante, Michael J. West, Gian Luigi Granato
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Contradictory results have been reported on the time evolution of the alignment between clusters and their Brightest Cluster Galaxy (BCG). We study this topic by analyzing cosmological hydro-simulations of 24 massive clusters with $M_{200}|_{z=0} \gt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::300022ee16edda056f2eaf55e14d2de9
https://academic.oup.com/mnras/article/495/2/2436/5841296
https://academic.oup.com/mnras/article/495/2/2436/5841296
Autor:
Giuseppe Murante, Eda Gjergo, C. Ragone-Figueroa, L. Tornatore, Gian Luigi Granato, Stefano Borgani
Publikováno v:
Monthly Notices of the Royal Astronomical Society
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We implement a state-of-the-art treatment of the processes affecting the production and Interstellar Medium (ISM) evolution of carbonaceous and silicate dust grains within SPH simulations. We trace the dust grain size distribution by means of a two-s
Autor:
Pasquale Mazzotta, C. Ragone-Figueroa, Susana Planelles, D. Fabjan, Massimo Gaspari, Giuseppe Murante, Klaus Dolag, Gian Luigi Granato, Stefano Borgani, Elena Rasia, N. Truong, A. M. Beck, Lisa K. Steinborn, Veronica Biffi
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity, gas mass, X-ray temperature, and $Y_{X}$. Three sets of simulations ar
Akademický článek
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