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Dynamics of M87 jet
Published online by Cambridge University Press: 28 October 2024
Abstract
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Flows originating from black hole magnetospheres via Blandford-Znajek (BZ) process start highly relativistically, with very large Lorentz factors γ01, imprinted into the flow during pair production within the gaps. As a result, BZ-driven outflows would produce spine-brightened images, contrary to observations of the edge-brightened jet in M87. We conclude that M87 jet is not BZ-driven.
Keywords
- Type
- Contributed Paper
- Information
- Proceedings of the International Astronomical Union , Volume 19 , Symposium S378: Black Hole Winds at All Scales , December 2023 , pp. 8 - 11
- Copyright
- © The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union
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