Hostname: page-component-6587cd75c8-rlsgg Total loading time: 0 Render date: 2025-04-23T22:44:59.187Z Has data issue: false hasContentIssue false

Dynamics of M87 jet

Published online by Cambridge University Press:  28 October 2024

Maxim Lyutikov*
Affiliation:
Department of Physics and Astronomy, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907-2036

Abstract

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.

Type
Contributed Paper
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable

References

Acciari, et al. 2008, ApJ, 679, 397 CrossRefGoogle Scholar
Aharonian, et al. 2005, A&A, 442, 895 Google Scholar
Aharonian, et al. 2006, Science, 314, 1424 CrossRefGoogle Scholar
Bicknell, G. V., & Begelman, M. C. 1996, ApJ, 467, 597 CrossRefGoogle Scholar
Blandford, et al. 2019, ARAA, 57, 467 CrossRefGoogle Scholar
Blandford, R. D., & Payne, D. G. 1982, MNRAS, 199, 883 CrossRefGoogle Scholar
Blandford, R. D., & Znajek, R. L. 1977, MNRAS, 179, 433 CrossRefGoogle Scholar
Kim, , 2018, A&A, 616, A188 Google Scholar
Nakamura, M., & Asada, K. 2013, ApJ, 775, 118 CrossRefGoogle Scholar
Rieger, F. M., & Aharonian, F. A. 2008, A&A, 479, L5 Google Scholar