Hydrodynamical Simulations of Recollimation Shocks within Relativistic Astrophysical Jets
Hydrodynamical Simulations of Recollimation Shocks within Relativistic Astrophysical Jets
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Basel: MDPI AG
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English
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Basel: MDPI AG
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Astrophysical jets launched from active galactic nuclei can remain tightly collimated over large distances due, in part, to recollimation shocks. Formed within the jets due to their supersonic nature, recollimation shocks are predicted to leave signatures in the observed radio emission due to magnetic flux freezing and the geometric relationship be...
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Hydrodynamical Simulations of Recollimation Shocks within Relativistic Astrophysical Jets
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TN_cdi_doaj_primary_oai_doaj_org_article_fbfeeb6cf47546d7b6872776e2f18e79
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_fbfeeb6cf47546d7b6872776e2f18e79
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ISSN
2075-4434
E-ISSN
2075-4434
DOI
10.3390/galaxies6020053
