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

@article{MillerJones2019ARC,
  title={A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni},
  author={James C. A. Miller-Jones and Alexandra J. Tetarenko and Gregory R. Sivakoff and Matthew J. Middleton and Diego Altamirano and G. E. Anderson and Tomaso M. Belloni and Robert P. Fender and Peter G. Jonker and Elmar K{\"o}rding and Hans A. Krimm and Dipankar Maitra and Sera B. Markoff and Simone Migliari and Kunal P. Mooley and Michael P. Rupen and David M. Russell and Thomas D. Russell and Craig L. Sarazin and Roberto Soria and Valeriu Tudose},
  journal={Nature},
  year={2019},
  volume={569},
  pages={374-377}
}
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 precession1 due to frame-dragging effects that occur when the black-hole spin axis is misaligned with the orbital plane of its companion star2. Recently, theoretical… 

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