2-D MHD Configurations for Accretion Disks Around Magnetized Stars
classification
🌌 astro-ph.SR
astro-ph.HE
keywords
accretionaroundmagnetizedastrophysicalballooningbasiccompactcomparison
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We discuss basic features of steady accretion disk morphology around magnetized compact astrophysical objects. A comparison between the standard model of accretion based on visco-resistive MHD and the plasma instabilities, like ballooning modes, triggered by very low value of resistivity, is proposed.
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