Local models of astrophysical discs
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DOI: 10.1093/mnras/stx2038
Abstract: Local models of gaseous accretion discs have been successfully employed for decades to describe an assortment of small-scale phenomena, from instabilities and turbulence, to dust dynamics and planet formation. For the most part, they have… read more here.
Keywords: models astrophysical; astrophysical discs; local models;