Measuring the density structure of an accretion hot spot
Measuring the density structure of an accretion hot spot
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Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
Magnetospheric accretion models predict that matter from protoplanetary disks accretes onto stars via funnel flows, which follow stellar magnetic field lines and shock on the stellar surfaces
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, leaving hot spots with density gradients
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. Previous work has provided observational evidence of varying density in hot s...
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Full title
Measuring the density structure of an accretion hot spot
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TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_8410598
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_8410598
Other Identifiers
ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-021-03751-5