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of 160
pro vyhledávání: '"L. Tornatore"'
Akademický článek
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Akademický článek
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Autor:
Gian Luigi Granato, Fabrizio Brighenti, Pierluigi Monaco, Giuseppe Murante, Andrea Lapi, Alessandro Bressan, Stefano Borgani, Milena Valentini, L. Tornatore
We present simulations of galaxy formation, based on the GADGET-3 code, in which a sub-resolution model for star formation and stellar feedback is interfaced with a new model for AGN feedback. Our sub-resolution model describes a multiphase ISM, acco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb5ae139c422b46cd980d8c641aed394
http://hdl.handle.net/11585/743824
http://hdl.handle.net/11585/743824
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:
Klaus Dolag, L. Tornatore, Nicolas Clerc, Didier Barret, F. Pajot, Stefano Ettori, Etienne Pointecouteau, P. Peille, V. Biffi, Esra Bulbul, Edoardo Cucchetti, E. Rasia, Thomas Dauser, Jörn Wilms, Stefano Borgani, Mauro Roncarelli, F. Mernier, Massimo Gaspari
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A90. ⟨10.1051/0004-6361/202038638⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A90. ⟨10.1051/0004-6361/202038638⟩
The chemical enrichment of the Universe at all scales is related to stellar winds and explosive supernovae phenomena. Metals produced by stars and later spread at the mega-parsec scale through the intra-cluster medium (ICM) become a fossil record of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7652c017443218dbecc26fe7e54c9217
https://hal.archives-ouvertes.fr/hal-02939899
https://hal.archives-ouvertes.fr/hal-02939899
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ecf3c7a68893c42e7aed5371b38f8eed
https://doi.org/10.1093/mnras/sty1564
https://doi.org/10.1093/mnras/sty1564
Autor:
Manolis Katevenis, A. Ragagnin, L. Tornatore, Igor Coretti, Giuliano Taffoni, Sara Bertocco, Fabien Chaix, Manolis Marazakis, Renato Panchieri, Manolis Plumidis, Gino Perna, David Goz
Publikováno v:
eScience
The increasing amount of data produced in Astronomy by observational studies and the size of theoretical problems to be tackled in the next future pushes the need of HPC (High Performance Computing) resources towards the "Exascale". The HPC sector is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0c717072d05645207c896c210bb74432
https://doi.org/10.1109/escience.2019.00052
https://doi.org/10.1109/escience.2019.00052
Autor:
Alessandro Bressan, Pierluigi Monaco, Stefano Borgani, Giuseppe Murante, Milena Valentini, L. Tornatore
We perform a suite of cosmological hydrodynamical simulations of disc galaxies, with zoomed-in initial conditions leading to the formation of a halo of mass $M_{\rm halo, \, DM} \simeq 2 \cdot 10^{12}$ M$_{\odot}$ at redshift $z=0$. These simulations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce7597d4bae64ee48245178395725821
http://hdl.handle.net/20.500.11767/108195
http://hdl.handle.net/20.500.11767/108195
Akademický článek
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Autor:
Alessandro Bressan, Léo Girardi, Giuseppe Murante, Milena Valentini, L. Tornatore, Stefano Borgani
State-of-the-art cosmological hydrodynamical simulations have star particles with typical mass between $\sim 10^8$ and $\sim 10^3$ M$_{\odot}$ according to resolution, and treat them as simple stellar populations. On the other hand, observations in n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6903c00e4c5669cd612293e93df52fe7
http://hdl.handle.net/11368/2930137
http://hdl.handle.net/11368/2930137