Cosmic magnetism evolution using cosmological simulations

The Intergalactic Medium (IGM) is the region comprising the environment between the galaxies. Gamma-ray observations have provided lower limits to IGM magnetic fields of the order of ≳10–16 G. Magnetic fields are continuously ejected from galaxies by jets and galactic winds. However, the origin and...

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Veröffentlicht in:	Proceedings of the International Astronomical Union 2020-03, Vol.15 (S359), p.175-177
Hauptverfasser:	Adduci Faria, Stela, de Gouveia Dal Pino, Elisabete M., Barai, Paramita
Format:	Artikel
Sprache:	eng
Schlagworte:	Amplification Astronomy Contributed Papers Equipartition theorem Fluid flow Galactic evolution Galactic winds Galaxies Gamma rays Halos Intergalactic media Magnetic fields Magnetism Magnetohydrodynamic turbulence Magnetohydrodynamics Simulation
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