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A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni

A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2239953393

A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni

About this item

Full title

A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2019-06

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them should be affected by the dynamics of the flow, which in accreting stellar-mass black holes has shown increasing evidence for precession due to fra...

Alternative Titles

Full title

A rapidly-changing jet orientation in the stellar-mass black hole V404 Cygni

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2239953393

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2239953393

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1906.05400

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