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

Journal: Nature

Published: 2019-04-29

DOI: 10.1038/s41586-019-1152-0

Affiliations: 24

Authors: 21

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Institutions FC
International Centre for Radio Astronomy Research (ICRAR), Australia 0.11
School of Physics and Astronomy (P&A), Soton, United Kingdom (UK) 0.10
Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), RU, Netherlands 0.07
Department of Physics, U of A, Canada 0.07
Anton Pannekoek Institute for Astronomy (API), UvA, Netherlands 0.07
Oxford Sub-Department of Astrophysics, United Kingdom (UK) 0.06
NRC Herzberg Astronomy and Astrophysics Research Centre (NRC Herzberg), Canada 0.05
Department of Astronomy, UVA, United States of America (USA) 0.05
New York University Abu Dhabi (NYUAD), United Arab Emirates 0.05
Institute of Space Science (ISS), Romania 0.05
INAF - Astronomical Observatory of Brera (OAB) - Merate, Italy 0.05
Department of Physics, Wheaton College - Norton, United States of America (USA) 0.02
Department of Astronomy, Wheaton College - Norton, United States of America (USA) 0.02
East Asian Observatory (EAO), United States of America (USA) 0.02
GRavitation and AstroParticle Physics Amsterdam (GRAPPA), UvA, Netherlands 0.02
SRON Netherlands Institute for Space Research, Netherlands 0.02
Institute of Cosmos Sciences (ICC), UB, Spain 0.02
National Science Foundation (NSF), United States of America (USA) 0.02
Universities Space Research Association (USRA), United States of America (USA) 0.02
X-ray Multi-Mirror Mission Science Operations Centre (XMM-Newton SOC), ESAC, Spain 0.02
NSF National Radio Astronomy Observatory (NRAO), United States of America (USA) 0.02
California Institute of Technology (Caltech), United States of America (USA) 0.02
School of Astronomy and Space Science, UCAS, China 0.02
Sydney Institute for Astronomy (SIfA), USYD, Australia 0.02

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