• DOI:10.1038/s41586-019-1152-0
Corpus ID: 139106116

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={J. Miller-Jones and A. J. Tetarenko and G. Sivakoff and M. Middleton and D. Altamirano and G. Anderson and T. Belloni and R. Fender and P. Jonker and E. K{\"o}rding and H. Krimm and D. Maitra and S. Markoff and S. Migliari and K. Mooley and M. Rupen and D. Russell and T. D. Russell and C. Sarazin and R. Soria and V. Tudose},
  journal={Nature},
  year={2019},
  volume={569},
  pages={374-377}
}

J. Miller-Jones, A. J. Tetarenko, +18 authors V. Tudose

Published 2019

Physics, Medicine

Nature

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… CONTINUE READING

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