Dynamics and high-energy emission of the flaring HST-1 knot in the M 87 jet-Reference-Cited by-同舟云学术

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Dynamics and high-energy emission of the flaring HST-1 knot in the M 87 jet

Published:2006-08-01 Issue:2 Volume:370 Page:981-992
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Stawarz L.,Aharonian F.,Kataoka J.,Ostrowski M.,Siemiginowska A.,Sikora M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/370/2/981/2912397/mnras0370-0981.pdf

Reference71 articles.

1. Is the giant radio galaxy M 87 a TeV gamma-ray emitter?

2. Are Centaurus A and M87 T[CLC]e[/CLC]V Gamma-Ray Sources?

3. Understanding the Kiloparsec-Scale Structure of M87

4. The radio to X-ray spectrum of the M87 jet and nucleus

5. Detection of Proper Motions in the M87 Jet

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1. HST-1 as a window into the energetics of the jet spine of M 87;Astronomy & Astrophysics;2023-09

2. Precession-induced Variability in AGN Jets and OJ 287;The Astrophysical Journal;2023-07-01

3. Interface instabilities in hydrodynamic relativistic jets;Monthly Notices of the Royal Astronomical Society;2023-01-16

4. Implications from the Velocity Profile of the M87 Jet: A Possibility of a Slowly Rotating Black Hole Magnetosphere;The Astrophysical Journal;2022-11-01

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