A noninteracting low-mass black hole–giant star binary system

@article{Thompson2019ANL,
  title={A noninteracting low-mass black hole–giant star binary system},
  author={T. A. Thompson and C. Kochanek and K. Stanek and C. Badenes and R. S. Post and T. Jayasinghe and D. Latham and A. Bieryla and G. A. Esquerdo and P. Berlind and M. L. Calkins and J. Tayar and L. Lindegren and J. A. Johnson and T. W. Holoien and K. Auchettl and K. Covey},
  journal={Science},
  year={2019},
  volume={366},
  pages={637 - 640}
}
  • T. A. Thompson, C. Kochanek, +14 authors K. Covey
  • Published 2019
  • Physics, Medicine
  • Science
  • A black hole hiding in a binary star As material falls toward a black hole, it heats up and emits x-rays. Almost all black holes are discovered by this x-ray emission. Thompson et al. observed light from a giant star that is Doppler shifted, indicating an orbit around a binary companion. The companion object must weigh more than 2.6 solar masses, but it emits no light, including x-rays. This indicates the presence of a black hole that is not currently consuming any material. There may be a… CONTINUE READING
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