Contribution to the angular momentum transport paradigm for accretion disks

We analyze the stationary configuration of a thin axisymmetric stellar accretion disk, neglecting non-linear terms in the plasma poloidal velocity components. We set up the Grad-Shafranov equation for the system, including the plasma differential rotation (according to the so-called co-rotation theo...

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Auteurs principaux: Giovanni Montani, Nakia Carlevaro
Format: article
Langue:EN
Publié: Elsevier 2021
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Accès en ligne:https://doaj.org/article/61660e424ce94f74ab635b260b9afcfb
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