Bent by baryons: the low-mass galaxy-halo relation - Test2 - elhamkhani - TriplyDB

Bent by baryons: the low-mass galaxy-halo relation

Bent by baryons: the low-mass galaxy-halo relation

http://www.wikidata.org/entity/Q56907945

about

A low pre-infall mass for the Carina dwarf galaxy from disequilibrium modelling.Modelling galaxy clustering: halo occupation distribution versus subhalo matching.Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo The galaxy population in cold and warm dark matter cosmologies Shaken and stirred: the Milky Way's dark substructures Size matters: abundance matching, galaxy sizes, and the Tully–Fisher relation in EAGLE Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations Reionization in sterile neutrino cosmologies The Copernicus Complexio: a high-resolution view of the small-scale Universe The apostle project: Local Group kinematic mass constraints and simulation candidate selection The chosen few: the low-mass haloes that host faint galaxies The Copernicus Complexio: statistical properties of warm dark matter haloes The Milky Way system in Λ cold dark matter cosmological simulations The unexpected diversity of dwarf galaxy rotation curves Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations Too small to succeed: the difficulty of sustaining star formation in low-mass haloes On the connection between the metal-enriched intergalactic medium and galaxies: an O vi–galaxy cross-correlation study atz< 1 Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass–metallicity relation

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Bent by baryons: the low-mass galaxy-halo relation

http://www.wikidata.org/entity/Q56907945

description

article

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im März 2015 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована в березні 2015

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name

Bent by baryons: the low-mass galaxy-halo relation

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Bent by baryons: the low-mass galaxy-halo relation

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type

label

Bent by baryons: the low-mass galaxy-halo relation

@en

Bent by baryons: the low-mass galaxy-halo relation

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prefLabel

Bent by baryons: the low-mass galaxy-halo relation

@en

Bent by baryons: the low-mass galaxy-halo relation

@nl

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Monthly Notices of the Royal Astronomical Society

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Bent by baryons: the low-mass galaxy-halo relation

@en

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Carlos S. Frenk

http://www.w3.org/2001/XMLSchema#string

Ian G. McCarthy

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Julio F. Navarro

http://www.w3.org/2001/XMLSchema#string

Michelle Furlong

http://www.w3.org/2001/XMLSchema#string

Richard G. Bower

http://www.w3.org/2001/XMLSchema#string

Till Sawala

http://www.w3.org/2001/XMLSchema#string

Yan Qu

http://www.w3.org/2001/XMLSchema#string

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Planck 2013 results. XVI. Cosmological parameters

Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering

The evolution of large-scale structure in a universe dominated by cold dark matter

The physics driving the cosmic star formation history

The EAGLE project: simulating the evolution and assembly of galaxies and their environments

The abundance of (not just) dark matter haloes

The Aquila comparison project: the effects of feedback and numerical methods on simulations of galaxy formation

The SPLASH survey: spectroscopy of 15 M31 dwarf spheroidal satellite galaxies

The effects of photoionization on galaxy formation - II. Satellite galaxies in the Local Group

Dark and luminous matter in THINGS dwarf galaxies

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2941–2947

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scholarly article

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10.1093/MNRAS/STU2753

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3

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448

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Matthieu Schaller

Robert A. Crain

Claudio Dalla Vecchia

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2015-03-05T00:00:00Z

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1404.3724

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2015MNRAS.448.2941S

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