What is it about?

The story of how super-massive black holes in the nuclei of many galaxies eject excess matter in the form at powerful winds moving at one tenth the velocity of light.

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Why is it important?

Such powerful winds will clear away gas from the central bulge of the host galaxy, thereby limiting star formation and the growth of the black hole.

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This page is a summary of: X-ray astronomy and Eddington winds, Astronomy & Geophysics, December 2017, Oxford University Press (OUP),
DOI: 10.1093/astrogeo/atx215.
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