How supernova feedback turns dark matter cusps into cores
about
Cold dark matter: Controversies on small scalesStrongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago.Bridging the gap: from massive stars to supernovae.Stellar feedback as the origin of an extended molecular outflow in a starburst galaxy.Understanding the core-halo relation of quantum wave dark matter from 3D simulations.Galaxy structure from multiple tracers – II. M87 from parsec to megaparsec scalesAdaptive techniques for clustered N-body cosmological simulationsThe impact of baryonic physics on the structure of dark matter haloes: the view from the FIRE cosmological simulationsCore formation in dwarf haloes with self-interacting dark matter: no fine-tuning necessaryDark matter annihilation and decay in dwarf spheroidal galaxies: the classical and ultrafaint dSphsThe Milky Way's stellar disk. Mapping and modeling the Galactic diskKnown unknowns of dark matter annihilation over cosmic timeThe core–cusp problem: a matter of perspectiveComparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar haloAddressing the too big to fail problem with baryon physics and sterile neutrino dark matterParticle tagging and its implications for stellar population dynamicsSatellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matterThe Copernicus Complexio: a high-resolution view of the small-scale UniverseDark matter annihilation radiation in hydrodynamic simulations of Milky Way haloesThe effect of baryons on the inner density profiles of rich clustersBaryon effects on the internal structure of ΛCDM haloes in the EAGLE simulationsSurface photometry of brightest cluster galaxies and intracluster stars in ΛCDMThe properties of warm dark matter haloesGalactic accretion and the outer structure of galaxies in the CDM modelThe abundance of (not just) dark matter haloesDark matter halo merger histories beyond cold dark matter – I. Methods and application to warm dark matterDark matter and cosmic structureFrom cusps to cores: a stochastic modelAGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxiesBlowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitorCold dark matter heats upAbundance of field galaxiesThe inner structure of haloes in cold+warm dark matter modelsToo small to succeed: the difficulty of sustaining star formation in low-mass haloesNovel Adaptive softening for collisionlessN-body simulations: eliminating spurious haloesConstraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshiftsSmall scale clustering of late forming dark matterExtragalactic gamma-ray signal from dark matter annihilation: an appraisalConstraints on large-scale dark acoustic oscillations from cosmologyCosmological simulations with self-interacting dark matter – I. Constant-density cores and substructure
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How supernova feedback turns dark matter cusps into cores
description
im März 2012 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в березні 2012
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name
How supernova feedback turns dark matter cusps into cores
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How supernova feedback turns dark matter cusps into cores
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type
label
How supernova feedback turns dark matter cusps into cores
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How supernova feedback turns dark matter cusps into cores
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prefLabel
How supernova feedback turns dark matter cusps into cores
@en
How supernova feedback turns dark matter cusps into cores
@nl
P2860
P1476
How supernova feedback turns dark matter cusps into cores
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P2093
Fabio Governato
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P304
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10.1111/J.1365-2966.2012.20571.X
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P577
2012-03-15T00:00:00Z
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P818
P819
2012MNRAS.421.3464P