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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Scope and Contents
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...
Alternative Titles
Full title
Measuring the density structure of an accretion hot spot
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Record Identifier
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
