Log in to save to my catalogue

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

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

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2217470837

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

About this item

Full title

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

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2019-05, Vol.569 (7756), p.374-377

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

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 are expected to be affected by the dynamics of the flow, which for accreting stellar-mass black holes has shown evidence for precession
1
due...

Alternative Titles

Full title

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

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_2217470837

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2217470837

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/s41586-019-1152-0

How to access this item