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Measuring the density structure of an accretion hot spot

Measuring the density structure of an accretion hot spot

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_8410598

Measuring the density structure of an accretion hot spot

About this item

Full title

Measuring the density structure of an accretion hot spot

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2021-09, Vol.597 (7874), p.41-44

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

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
1

3
, leaving hot spots with density gradients
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6
. 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

Identifiers

Primary Identifiers

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

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