A three-phase amplification of the cosmic magnetic field in galaxies

A three-phase amplification of the cosmic magnetic field in galaxies

Arguably the main challenge of galactic magnetism studies is to explain how the interstellar medium of galaxies reaches energetic equipartition despite the extremely weak cosmic primordial magnetic fields that are originally predicted to thread the inter-galactic medium. Previous numerical studies o...

Bibliografski detalji
Glavni autori:	Martin-Alvarez, S, Devriendt, J, Slyz, A, Teyssier, R
Format:	Journal article
Izdano:	Oxford University Press 2018

Slični predmeti

Unraveling the origin of magnetic fields in galaxies
od: Martin-Alvarez, S, i dr.
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How primordial magnetic fields shrink galaxies
od: Martin-Alvarez, S, i dr.
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How the cosmic web induces intrinsic alignments of galaxies
od: Codis, S, i dr.
Izdano: (2016)

Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies
od: Martin-Alvarez, S, i dr.
Izdano: (2022)

Connecting the cosmic web to the spin of dark halos: implications for galaxy formation
od: Codis, S, i dr.
Izdano: (2012)

Dwarf galaxies as a probe of a primordially magnetized Universe
od: Sanati, M, i dr.
Izdano: (2024)

The Horizon-AGN simulation: evolution of galaxy properties over cosmic time
od: Kaviraj, S, i dr.
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How to quench a dwarf galaxy: The impact of inhomogeneous reionization on dwarf galaxies and cosmic filaments
od: Katz, H, i dr.
Izdano: (2020)

Galaxy orientation with the cosmic web across cosmic time
od: Codis, S, i dr.
Izdano: (2018)

Intrinsic alignment of simulated galaxies in the cosmic web: implications for weak lensing surveys
od: Codis, S, i dr.
Izdano: (2015)

Introducing SPHINX-MHD: the impact of primordial magnetic fields on the first galaxies, reionization, and the global 21-cm signal
od: Katz, H, i dr.
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Magnetic field amplification by cosmic rays in supernova remnants
od: Schure, K, i dr.
Izdano: (2012)

Amplification of perpendicular and parallel magnetic fields by cosmic ray currents
od: Matthews, J, i dr.
Izdano: (2017)

A Galaxy in the Making
od: Slyz, A, i dr.
Izdano: (2010)

The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
od: Kraljic, K, i dr.
Izdano: (2019)

Momentum deposition of supernovae with cosmic rays
od: Montero, FR, i dr.
Izdano: (2022)

Momentum deposition of supernovae with cosmic rays
od: Montero, FR, i dr.
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Modeling high-redshift galaxies: what can we learn from high and ultra-high resolution hydrodynamical simulations?
od: Devriendt, J, i dr.
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Impact of star formation models on the growth of galaxies at high redshifts
od: Kang, C, i dr.
Izdano: (2024)

The formation of cores in galaxies across cosmic time – the existence of cores is not in tension with the ΛCDM paradigm
od: Jackson, RA, i dr.
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Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
od: Bell, A
Izdano: (2004)

The nonlinear amplification of magnetic fields by cosmic rays at supernova remnant shocks
od: Reville, B, i dr.
Izdano: (2006)

Non-linear amplification of a magnetic field driven by cosmic ray streaming
od: Lucek, S, i dr.
Izdano: (2000)

Non-linear amplification of a magnetic field driven by cosmic ray streaming
od: Lucek, S, i dr.
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How do galaxies build up their spin in the cosmic web?
od: Welker, C, i dr.
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The impact of ISM turbulence, clustered star formation and feedback on galaxy mass assembly through cold flows and mergers
od: Powell, L, i dr.
Izdano: (2010)

The impact of ISM turbulence, clustered star formation and feedback on galaxy mass assembly through cold flows and mergers
od: Powell, L, i dr.
Izdano: (2011)

A Model for Cosmic Magnetic Field Amplification: Effects of Pressure Anisotropy Perturbations
od: Ji-Hoon Ha
Izdano: (2024-12-01)

Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
od: Bell, A, i dr.
Izdano: (2019)

Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
od: Bell, A, i dr.
Izdano: (2001)

Galaxy evolution in the metric of the Cosmic Web
od: Kraljic, K, i dr.
Izdano: (2017)

Star Formation in Viscous Galaxy Disks
od: Slyz, A, i dr.
Izdano: (2000)

The limited role of galaxy mergers in driving stellar mass growth over cosmic time
od: Martin, G, i dr.
Izdano: (2017)

Inferring dark matter halo properties for H i-selected galaxies
od: Yasin, T, i dr.
Izdano: (2023)

The information on halo properties contained in spectroscopic observations of late-type galaxies
od: Yasin, T, i dr.
Izdano: (2023)

The information on halo properties contained in spectroscopic observations of late-type galaxies
od: Yasin, T, i dr.
Izdano: (2022)

Implications of strong intergalactic magnetic fields for ultrahigh-energy cosmic-ray astronomy
od: Batista, R, i dr.
Izdano: (2017)

Forming stars on a viscous timescale: the key to exponential stellar profiles in disk galaxies?
od: Slyz, A, i dr.
Izdano: (2001)

Cosmic-Ray Acceleration and Magnetic Fields in Galaxy Clusters and Beyond: Insights from Radio Observations
od: Denis Wittor
Izdano: (2023-07-01)

Enhancing and inhibiting star formation: High-resolution simulation studies of the impact of cold accretion, mergers and feedback on individual massive galaxies
od: Powell, L, i dr.
Izdano: (2012)