Search Results - "Marinacci, Federico"

Simulating the interstellar medium and stellar feedback on a moving mesh: implementation and isolated galaxies by Marinacci, Federico, Sales, Laura V, Vogelsberger, Mark, Torrey, Paul, Springel, Volker

“…ABSTRACT We introduce the Stars and MUltiphase Gas in GaLaxiEs – SMUGGLE model, an explicit and comprehensive stellar feedback model for the moving-mesh code…”
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Resolving small-scale cold circumgalactic gas in TNG50 by Nelson, Dylan, Sharma, Prateek, Pillepich, Annalisa, Springel, Volker, Pakmor, Rüdiger, Weinberger, Rainer, Vogelsberger, Mark, Marinacci, Federico, Hernquist, Lars

“…ABSTRACT We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to explore the properties and origin of cold circumgalactic medium…”
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Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies by Zinger, Elad, Pillepich, Annalisa, Nelson, Dylan, Weinberger, Rainer, Pakmor, Rüdiger, Springel, Volker, Hernquist, Lars, Marinacci, Federico, Vogelsberger, Mark

“…ABSTRACT Supermassive black holes (SMBHs) that reside at the centres of galaxies can inject vast amounts of energy into the surrounding gas and are thought to…”
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First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback by Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Pakmor, Rüdiger, Weinberger, Rainer, Genel, Shy, Torrey, Paul, Vogelsberger, Mark, Marinacci, Federico, Hernquist, Lars

“…Abstract We present the new TNG50 cosmological, magnetohydrodynamical simulation – the third and final volume of the IllustrisTNG project. This simulation…”
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Simulating the dust content of galaxies: successes and failures by McKinnon, Ryan, Torrey, Paul, Vogelsberger, Mark, Hayward, Christopher C., Marinacci, Federico

“…Abstract We present full-volume cosmological simulations, using the moving-mesh code arepo to study the coevolution of dust and galaxies. We extend the dust…”
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Disruption of giant molecular clouds and formation of bound star clusters under the influence of momentum stellar feedback by Li, Hui, Vogelsberger, Mark, Marinacci, Federico, Gnedin, Oleg Y

“…Abstract Energetic feedback from star clusters plays a pivotal role in shaping the dynamical evolution of giant molecular clouds (GMCs). To study the effects…”
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First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium by Naiman, Jill P, Pillepich, Annalisa, Springel, Volker, Ramirez-Ruiz, Enrico, Torrey, Paul, Vogelsberger, Mark, Pakmor, Rüdiger, Nelson, Dylan, Marinacci, Federico, Hernquist, Lars, Weinberger, Rainer, Genel, Shy

“…Abstract The distribution of elements in galaxies provides a wealth of information about their production sites and their subsequent mixing into the…”
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First results from the IllustrisTNG simulations: radio haloes and magnetic fields by Marinacci, Federico, Vogelsberger, Mark, Pakmor, Rüdiger, Torrey, Paul, Springel, Volker, Hernquist, Lars, Nelson, Dylan, Weinberger, Rainer, Pillepich, Annalisa, Naiman, Jill, Genel, Shy

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First results from the IllustrisTNG simulations: matter and galaxy clustering by Springel, Volker, Pakmor, Rüdiger, Pillepich, Annalisa, Weinberger, Rainer, Nelson, Dylan, Hernquist, Lars, Vogelsberger, Mark, Genel, Shy, Torrey, Paul, Marinacci, Federico, Naiman, Jill

“…Abstract Hydrodynamical simulations of galaxy formation have now reached sufficient volume to make precision predictions for clustering on cosmologically…”
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First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies by Pillepich, Annalisa, Nelson, Dylan, Hernquist, Lars, Springel, Volker, Pakmor, Rüdiger, Torrey, Paul, Weinberger, Rainer, Genel, Shy, Naiman, Jill P, Marinacci, Federico, Vogelsberger, Mark

“…Abstract The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations of galaxy formation performed with the arepo code and…”
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The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics by Donnari, Martina, Pillepich, Annalisa, Nelson, Dylan, Vogelsberger, Mark, Genel, Shy, Weinberger, Rainer, Marinacci, Federico, Springel, Volker, Hernquist, Lars

“…Abstract We select galaxies from the IllustrisTNG hydrodynamical simulations ($M_{\rm stars}\gt 10^9 \, {\rm M}_\odot$ at 0 ≤ z ≤ 2) and characterize the…”
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Effects of simulated cosmological magnetic fields on the galaxy population by Marinacci, Federico, Vogelsberger, Mark

“…We investigate the effects of varying the intensity of the primordial magnetic seed field on the global properties of the galaxy population in ideal…”
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The evolution of the mass–metallicity relation and its scatter in IllustrisTNG by Torrey, Paul, Vogelsberger, Mark, Marinacci, Federico, Pakmor, Rüdiger, Springel, Volker, Nelson, Dylan, Naiman, Jill, Pillepich, Annalisa, Genel, Shy, Weinberger, Rainer, Hernquist, Lars

“…ABSTRACT The coevolution of galaxies and their metal content serves as an important test for galaxy feedback models. We analyse the distribution and evolution…”
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The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation by Genel, Shy, Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Pakmor, Rüdiger, Weinberger, Rainer, Hernquist, Lars, Naiman, Jill, Vogelsberger, Mark, Marinacci, Federico, Torrey, Paul

“…Abstract We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the IllustrisTNG simulation suite. Observational qualitative…”
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The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations by Rodriguez-Gomez, Vicente, Snyder, Gregory F, Lotz, Jennifer M, Nelson, Dylan, Pillepich, Annalisa, Springel, Volker, Genel, Shy, Weinberger, Rainer, Tacchella, Sandro, Pakmor, Rüdiger, Torrey, Paul, Marinacci, Federico, Vogelsberger, Mark, Hernquist, Lars, Thilker, David A

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The physical origins and dominant emission mechanisms of Lyman alpha haloes: results from the TNG50 simulation in comparison to MUSE observations by Byrohl, Chris, Nelson, Dylan, Behrens, Christoph, Kostyuk, Ivan, Glatzle, Martin, Pillepich, Annalisa, Hernquist, Lars, Marinacci, Federico, Vogelsberger, Mark

“…ABSTRACT Extended Lyman alpha emission is now commonly detected around high-redshift galaxies through stacking and even on individual basis. Despite recent…”
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Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing by Donnari, Martina, Pillepich, Annalisa, Joshi, Gandhali D, Nelson, Dylan, Genel, Shy, Marinacci, Federico, Rodriguez-Gomez, Vicente, Pakmor, Rüdiger, Torrey, Paul, Vogelsberger, Mark, Hernquist, Lars

“…ABSTRACT We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched galaxies vary across different environments and cosmic time,…”
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Baryons in the Cosmic Web of IllustrisTNG – I: gas in knots, filaments, sheets, and voids by Martizzi, Davide, Vogelsberger, Mark, Artale, Maria Celeste, Haider, Markus, Torrey, Paul, Marinacci, Federico, Nelson, Dylan, Pillepich, Annalisa, Weinberger, Rainer, Hernquist, Lars, Naiman, Jill, Springel, Volker

“…ABSTRACT We analyse the IllustrisTNG simulations to study the mass, volume fraction, and phase distribution of gaseous baryons embedded in the knots,…”
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Formation and evolution of young massive clusters in galaxy mergers: the SMUGGLE view by Li, Hui, Vogelsberger, Mark, Bryan, Greg L, Marinacci, Federico, Sales, Laura V, Torrey, Paul

“…ABSTRACT Galaxy mergers are known to host abundant young massive cluster (YMC) populations, whose formation mechanism is still not well-understood. Here, we…”
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Ingredients for 21 cm Intensity Mapping by Villaescusa-Navarro, Francisco, Genel, Shy, Castorina, Emanuele, Obuljen, Andrej, Spergel, David N., Hernquist, Lars, Nelson, Dylan, Carucci, Isabella P., Pillepich, Annalisa, Marinacci, Federico, Diemer, Benedikt, Vogelsberger, Mark, Weinberger, Rainer, Pakmor, Rüdiger

“…Current and upcoming radio telescopes will map the spatial distribution of cosmic neutral hydrogen (H i) through its 21 cm emission. In order to extract the…”
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