Magnetohydrodynamic properties of extragalactic jets
The theory that magnetic fields are instrumental in the formation and propagation of jets in active galactic nuclei dates back four decades. Despite a recent growing consensus on this notion stemming from the results of numerical simulations of magnetohydrodynamic (MHD) flows near black holes, the p...
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| Published in | Astrophysics and space science Vol. 336; no. 1; pp. 15 - 19 |
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| Main Authors | , , |
| Format | Journal Article |
| Language | English |
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Dordrecht
Springer Netherlands
01.11.2011
Springer Nature B.V |
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| Abstract | The theory that magnetic fields are instrumental in the formation and propagation of jets in active galactic nuclei dates back four decades. Despite a recent growing consensus on this notion stemming from the results of numerical simulations of magnetohydrodynamic (MHD) flows near black holes, the precise dynamical role of magnetic fields in observed parsec and kiloparsec jets remains uncertain. Some of the unanswered fundamental questions about extragalactic jets include the location where the flow becomes relativistic and where acceleration and collimation terminate, as well as the specifics of how the flow interacts with the ISM. Such observed properties as superluminal motions and wiggled structures based on numerical simulations to constitute the foundation of an MHD paradigm for extragalactic jets. We particularly focus our attention to the M87 jet, which is one of the best candidates to investigate relativistic outflows in extragalactic system. |
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| AbstractList | The theory that magnetic fields are instrumental in the formation and propagation of jets in active galactic nuclei dates back four decades. Despite a recent growing consensus on this notion stemming from the results of numerical simulations of magnetohydrodynamic (MHD) flows near black holes, the precise dynamical role of magnetic fields in observed parsec and kiloparsec jets remains uncertain. Some of the unanswered fundamental questions about extragalactic jets include the location where the flow becomes relativistic and where acceleration and collimation terminate, as well as the specifics of how the flow interacts with the ISM. Such observed properties as superluminal motions and wiggled structures based on numerical simulations to constitute the foundation of an MHD paradigm for extragalactic jets. We particularly focus our attention to the M87 jet, which is one of the best candidates to investigate relativistic outflows in extragalactic system. Issue Title: NEW DEVELOPMENTS IN HIGH ENERGY DENSITY LABORATORY ASTROPHYSICS. The theory that magnetic fields are instrumental in the formation and propagation of jets in active galactic nuclei dates back four decades. Despite a recent growing consensus on this notion stemming from the results of numerical simulations of magnetohydrodynamic (MHD) flows near black holes, the precise dynamical role of magnetic fields in observed parsec and kiloparsec jets remains uncertain. Some of the unanswered fundamental questions about extragalactic jets include the location where the flow becomes relativistic and where acceleration and collimation terminate, as well as the specifics of how the flow interacts with the ISM. Such observed properties as superluminal motions and wiggled structures based on numerical simulations to constitute the foundation of an MHD paradigm for extragalactic jets. We particularly focus our attention to the M87 jet, which is one of the best candidates to investigate relativistic outflows in extragalactic system.[PUBLICATION ABSTRACT] |
| Author | Nakamura, M. Meier, D. L. Garofalo, D. |
| Author_xml | – sequence: 1 givenname: M. surname: Nakamura fullname: Nakamura, M. email: nakamura@pha.jhu.edu organization: Department of Physics and Astronomy, Johns Hopkins University, Space Telescope Science Institute – sequence: 2 givenname: D. L. surname: Meier fullname: Meier, D. L. organization: Jet Propulsion Laboratory, California Institute of Technology – sequence: 3 givenname: D. surname: Garofalo fullname: Garofalo, D. organization: Jet Propulsion Laboratory, California Institute of Technology |
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| Keywords | Active galaxies MHD Jets galaxies Numerical methods |
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| Snippet | The theory that magnetic fields are instrumental in the formation and propagation of jets in active galactic nuclei dates back four decades. Despite a recent... Issue Title: NEW DEVELOPMENTS IN HIGH ENERGY DENSITY LABORATORY ASTROPHYSICS. The theory that magnetic fields are instrumental in the formation and propagation... |
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| SubjectTerms | Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Cosmology Fluid mechanics Jets Magnetic fields Numerical analysis Observations and Techniques Original Article Physics Physics and Astronomy Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Stars & galaxies |
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| Title | Magnetohydrodynamic properties of extragalactic jets |
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