State-of-the-art energetic and morphological modelling of the launching site of the M87 jet-Reference-Cited by-同舟云学术

State-of-the-art energetic and morphological modelling of the launching site of the M87 jet

Published:2021-11-04 Issue:1 Volume:6 Page:103-108
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Cruz-Osorio Alejandro^ORCID,Fromm Christian M.,Mizuno Yosuke^ORCID,Nathanail Antonios,Younsi Ziri,Porth Oliver,Davelaar Jordy^ORCID,Falcke Heino,Kramer Michael^ORCID,Rezzolla Luciano

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01506-w.pdf

Reference42 articles.

1. Kovalev, Y. Y., Lister, M. L., Homan, D. C. & Kellermann, K. I. The inner jet of the radio galaxy M87. Astrophys. J. Lett. 668, L27–L30 (2007).

2. Asada, K. & Nakamura, M. The structure of the M87 jet: a transition from parabolic to conical streamlines. Astrophys. J. Lett. 745, L28 (2012).

3. Walker, R. C., Hardee, P. E., Davies, F. B., Ly, C. & Junor, W. The structure and dynamics of the subparsec jet in M87 based on 50 VLBA observations over 17 years at 43 GHz. Astrophys. J. 855, 128 (2018).

4. Kim, J.-Y. et al. The limb-brightened jet of M87 down to the 7 Schwarzschild radii scale. Astron. Astrophys. 616, A188 (2018).

5. Blandford, R. D. & Znajek, R. L. Electromagnetic extraction of energy from Kerr black holes. Mon. Not. R. Astron. Soc. 179, 433–456 (1977).

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