Search Results - "DEKEL, Avishai"
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An analytic solution for the minimal bathtub toy model: challenges in the star formation history of high-z galaxies
Published in Monthly notices of the Royal Astronomical Society (01-11-2014)“…We study the minimal ‘bathtub’ toy model as a tool for capturing key processes of galaxy evolution and identifying robust successes and challenges in…”
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Compaction-driven black hole growth
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT We study the interplay between galaxy evolution and central black hole (BH) growth using the NewHorizon cosmological simulation. BH growth is slow…”
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NIHAO – XI. Formation of ultra-diffuse galaxies by outflows
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2017)“…Abstract We address the origin of ultra-diffuse galaxies (UDGs), which have stellar masses typical of dwarf galaxies but effective radii of Milky Way-sized…”
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Quenching of satellite galaxies at the outskirts of galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract We find, using cosmological simulations of galaxy clusters, that the hot X-ray emitting intracluster medium (ICM) enclosed within the outer accretion…”
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Instability of supersonic cold streams feeding galaxies – IV. Survival of radiatively cooling streams
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT We study the effects of Kelvin–Helmholtz Instability (KHI) on the cold streams that feed massive haloes at high redshift, generalizing our earlier…”
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Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets
Published in Monthly notices of the Royal Astronomical Society (01-07-2015)“…We use cosmological simulations to study a characteristic evolution pattern of high-redshift galaxies. Early, stream-fed, highly perturbed, gas-rich discs…”
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Gravitational quenching in massive galaxies and clusters by clumpy accretion
Published in Monthly notices of the Royal Astronomical Society (01-01-2008)“…We consider a simple gravitational heating mechanism for the long-term quenching of cooling flows and star formation in massive dark matter haloes hosting…”
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Formation of ultra-diffuse galaxies in the field and in galaxy groups
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)“…ABSTRACT We study ultra-diffuse galaxies (UDGs) in zoom in cosmological simulations, seeking the origin of UDGs in the field versus galaxy groups. We find that…”
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Radiative feedback and the low efficiency of galaxy formation in low-mass haloes at high redshift
Published in Monthly notices of the Royal Astronomical Society (01-08-2014)“…Any successful model of galaxy formation needs to explain the low rate of star formation in the small progenitors of today's galaxies. This inefficiency is…”
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10
Scaling relations and the fundamental line of the local group dwarf galaxies
Published in Monthly notices of the Royal Astronomical Society (11-11-2008)“…We study the scaling relations between global properties of dwarf galaxies in the local group. In addition to quantifying the correlations between pairs of…”
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SatGen: a semi-analytical satellite galaxy generator – I. The model and its application to Local-Group satellite statistics
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT We present a semi-analytical model of satellite galaxies, SatGen, which can generate large statistical samples of satellite populations for a host…”
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12
On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
Published in Monthly notices of the Royal Astronomical Society (01-09-2014)“…We present a simple toy model to understand what sets the scatter in star formation and metallicity of galaxies at fixed mass. According to this model, the…”
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Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
Published in The Astrophysical journal (01-05-2017)“…We study the evolution of the scaling relations that compare the effective density ( ) and core density ( kpc) to the stellar masses of star-forming galaxies…”
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The population of giant clumps in simulated high-z galaxies: in situ and ex situ migration and survival
Published in Monthly notices of the Royal Astronomical Society (01-10-2014)“…We study the properties of giant clumps and their radial gradients in high-z disc galaxies using AMR cosmological simulations. Our sample consists of 770…”
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The relationship between galaxy and dark matter halo size from z ∼ 3 to the present
Published in Monthly notices of the Royal Astronomical Society (11-01-2018)Get full text
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Evaluating galaxy dynamical masses from kinematics and jeans equilibrium in simulations
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT We provide prescriptions to evaluate the dynamical mass (Mdyn) of galaxies from kinematic measurements of stars or gas using analytic considerations…”
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3
Published in The Astrophysical journal (01-02-2018)“…Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists…”
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Properties of dark matter haloes as a function of local environment density
Published in Monthly notices of the Royal Astronomical Society (01-05-2017)Get full text
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On the origin of the galaxy star-formation-rate sequence: evolution and scatter
Published in Monthly notices of the Royal Astronomical Society (01-07-2010)“…We use a semi-analytic model for disk galaxies to explore the origin of the time evolution and small scatter of the galaxy SFR sequence – the tight correlation…”
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NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…We use ∼100 cosmological galaxy formation ‘zoom-in’ simulations using the smoothed particle hydrodynamics code gasoline to study the effect of baryonic…”
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