The detection of a discrete knot of particle emission from the active galaxy M81* reveals that black hole accretion is self-similar with regard to mass, producing the same knotty jets irrespective of black hole mass and accretion rate.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 12 print issues and online access
$209.00 per year
only $17.42 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
King, A. L. et al. Nature Phys. http://dx.doi.org/10.1038/nphys3724 (2016).
Merloni, A., Heinz, S. & Di Matteo, T. Mon. Not. R. Astron. Soc. 345, 1057–1076 (2003).
Falcke, H., Körding, E. & Markoff, S. Astron. Astrophys. 414, 895–903 (2004).
Done, C., Gierlinski, M. & Kubota, A. Astron. Astrophys. Rev. 15, 1–66 (2007).
Chatterjee, R. et al. Astrophys. J. 734, 43 (2011).
Markoff, S. et al. Astrophys. J. 681, 905–924 (2008).
Markoff, S. et al. Astrophys. J. 812, L25 (2015).
Martí-Vidal, I. et al. Astron. Astrophys. 533, A111 (2011).
McKinney, J. C., Tchekhovskoy, A. & Blandford, R. D. Mon. Not. R. Astron. Soc. 423, 3083–3117 (2012).
Fender, R., Belloni, T. & Gallo, E. Astrophys. Space Sci. 300, 1–13 (2005).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Gómez, J. More similar than knot. Nature Phys 12, 729–730 (2016). https://doi.org/10.1038/nphys3748
Published:
Issue Date:
DOI: https://doi.org/10.1038/nphys3748