Search Results - "Pakmor, Rüdiger"
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Resolving small-scale cold circumgalactic gas in TNG50
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to explore the properties and origin of cold circumgalactic medium…”
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First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…Abstract We present the new TNG50 cosmological, magnetohydrodynamical simulation – the third and final volume of the IllustrisTNG project. This simulation…”
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First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…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
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)Get full text
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First results from the IllustrisTNG simulations: matter and galaxy clustering
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…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
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…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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Evolution of cosmic ray electron spectra in magnetohydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (11-09-2019)“…ABSTRACT Cosmic ray (CR) electrons reveal key insights into the non-thermal physics of the interstellar medium (ISM), galaxies, galaxy clusters, and active…”
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The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT We investigate the impact of cosmic rays (CRs) and different modes of CR transport on the properties of Milky Way-mass galaxies in cosmological…”
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The dependence of cosmic ray-driven galactic winds on halo mass
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…Abstract Galactic winds regulate star formation in disc galaxies and help to enrich the circum-galactic medium. They are therefore crucial for galaxy…”
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The Progenitors of Calcium-strong Transients
Published in The Astrophysical journal (20-12-2019)“…A new class of faint, spectroscopically peculiar transients has emerged in the last decade. We term these events "calcium-strong transients" (CaSTs) because of…”
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Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT We compare the star-forming main sequence (SFMS) of galaxies – both integrated and resolved on 1 kpc scales – between the high-resolution TNG50…”
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The evolution of the mass–metallicity relation and its scatter in IllustrisTNG
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)“…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
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…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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Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…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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Ingredients for 21 cm Intensity Mapping
Published in The Astrophysical journal (20-10-2018)“…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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Improving the convergence properties of the moving-mesh code AREPO
Published in Monthly notices of the Royal Astronomical Society (01-01-2016)“…Accurate numerical solutions of the equations of hydrodynamics play an ever more important role in many fields of astrophysics. In this work, we reinvestigate…”
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The fraction of dark matter within galaxies from the IllustrisTNG simulations
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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Quenching and ram pressure stripping of simulated Milky Way satellite galaxies
Published in Monthly notices of the Royal Astronomical Society (21-07-2018)“…Abstract We present predictions for the quenching of star formation in satellite galaxies of the Local Group from a suite of 30 cosmological zoom simulations…”
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The local high-velocity tail and the Galactic escape speed
Published in Monthly notices of the Royal Astronomical Society (21-05-2019)“…Abstract We model the fastest moving ($v_{\rm tot} \gt 300 \, {\rm km}\, \, {\rm s}^{-1}$) local (D ≲ 3 kpc) halo stars using cosmological simulations and…”
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Dark matter halo shapes in the Auriga simulations
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…ABSTRACT We present shape measurements of Milky Way–sized dark matter haloes at redshift z = 0 in a suite of 30 zoom simulations from the Auriga project. We…”
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