United Theory of Planet Formation (I): Tandem Regime
United Theory of Planet Formation (I): Tandem Regime
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We have obtained a steady-state, 1-D model of the accretion disk of a protostar taking into account the magneto-rotational instability (MRI). We find that the disk is divided into an outer turbulent region (OTR), a MRI suppressed region (MSR), and an inner turbulent region (ITR). The outer turbulent region is fully turbulent because of MRI. However...
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Full title
United Theory of Planet Formation (I): Tandem Regime
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TN_cdi_proquest_journals_2075301009
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2075301009
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1601.05509
