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THE STRUCTURE OF THE M87 JET: A TRANSITION FROM PARABOLIC TO CONICAL STREAMLINES

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Asada, Keiichi, Nakamura, Masanori·2012·The Astrophysical Journal

Abstract

The structure of the M87 jet, from milliarcsecond to arcsecond scales, is extensively investigated, utilizing the images taken with the European VLBI Network, MERLIN, and Very Long Baseline Array. We discover that the jet maintains a parabolic streamline over a range in size scale equal to 10 5 times the Schwarzschild radius. The jet then transitions into a conical shape farther downstream. This suggests that the magnetohydrodynamic jet is initially subjected to the confinement by the external gas which is dominated by the gravitational influence of the supermassive black hole. Afterward the jet then freely expands with a conical shape. This geometrical transition indicates that the origin of the HST-1 complex may be a consequence of the overcollimation of the jet. Our result suggests that when even higher angular resolution is provided by a future submillimeter very long baseline interferometry experiments, we will be able to explore the origin of active galactic nucleus jets.

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Metadata

Authors
Asada, K., & Nakamura, M.
Venue
The Astrophysical Journal
Published
2012-01-11
Volume
745
Issue
2
Pages
L28
ISSN
  • 2041-8205 (ISSN-L)
  • 2041-8213
OpenAlex
W1973497701
Cited by
313
References
0
FWCI
9.39
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: THE STRUCTURE OF THE M87 JET: A TRANSITION FROM PARABOLIC TO CONICAL STREAMLINES. https://app.cochat.ai/papers/10.1088/2041-8205/745/2/l28
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Asada, K., & Nakamura, M. (2012). THE STRUCTURE OF THE M87 JET: A TRANSITION FROM PARABOLIC TO CONICAL STREAMLINES. The Astrophysical Journal. https://doi.org/10.1088/2041-8205/745/2/l28

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