Magnetohydrodynamic Production of Relativistic Jets
A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of light. In all cases, the central object is probably a neutron star or black hole and is either accreting material from other stars or is in the initial violent stages...
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| Published in | Science (American Association for the Advancement of Science) Vol. 291; no. 5501; pp. 84 - 92 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
Washington, DC
American Society for the Advancement of Science
05.01.2001
American Association for the Advancement of Science The American Association for the Advancement of Science |
| Subjects | |
| Online Access | Get full text |
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| Abstract | A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of light. In all cases, the central object is probably a neutron star or black hole and is either accreting material from other stars or is in the initial violent stages of formation. Supercomputer simulations of the production of relativistic jets have been based on a magnetohydrodynamic model, in which differential rotation in the system creates a magnetic coil that simultaneously expels and pinches some of the infalling material. The model may explain the basic features of observed jets, including their speed and amount of collimation, and some of the details in the behavior and statistics of different jet-producing sources. |
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| AbstractList | A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of light. In all cases, the central object is probably a neutron star or black hole and is either accreting material from other stars or is in the initial violent stages of formation. A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of light. In all cases, the central object is probably a neutron star or black hole and is either accreting material from other stars or is in the initial violent stages of formation. Supercomputer simulations of the production of relativistic jets have been based on a magnetohydrodynamic model, in which differential rotation in the system creates a magnetic coil that simultaneously expels and pinches some of the infalling material. The model may explain the basic features of observed jets, including their speed and amount of collimation, and some of the details in the behavior and statistics of different jet-producing sources. A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of tight. In all cases, the central object is probably a neutron star or black hole and is either accreting material from other stars or is in the initial violent stages of formation. Supercomputer simulations of the production of relativistic jets have been based on a magnetohydrodynamic model, in which differential rotation in the system creates a magnetic coil that simultaneously expels and pinches some of the infalling material The model may explain the basic features of observed jets, including their speed and amount of collimation, and some of the details in the behavior and statistics of different jet-producing sources. |
| Audience | Academic |
| Author | Uchida, Yutaka Koide, Shinji Meier, David L. |
| Author_xml | – sequence: 1 givenname: David L. surname: Meier fullname: Meier, David L. – sequence: 2 givenname: Shinji surname: Koide fullname: Koide, Shinji – sequence: 3 givenname: Yutaka surname: Uchida fullname: Uchida, Yutaka |
| BackLink | http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=857706$$DView record in Pascal Francis https://www.ncbi.nlm.nih.gov/pubmed/11141552$$D View this record in MEDLINE/PubMed |
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| ClassificationCodes | 8521300 |
| ContentType | Journal Article |
| Copyright | Copyright 2001 American Association for the Advancement of Science 2001 INIST-CNRS COPYRIGHT 2001 American Association for the Advancement of Science COPYRIGHT 2001 American Association for the Advancement of Science Copyright American Association for the Advancement of Science Jan 5, 2001 |
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| DOI | 10.1126/science.291.5501.84 |
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| Snippet | A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of light. In all cases, the... A number of astronomical systems have been discovered that generate collimated flows of plasma with velocities close to the speed of tight. In all cases, the... |
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| SubjectTerms | Accretion disks Astronomical objects Astronomy Astrophysics Black holes Earth, ocean, space Exact sciences and technology Fluid dynamics Fundamental aspects of astrophysics Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Jets Jets (Fluid dynamics) Kinetics Magnetic fields Magnetism Magnetohydrodynamics and plasmas Observations Quasars Relativistic jets Reviews Rotation Simulation Stars Supercomputers Supernovae |
| Title | Magnetohydrodynamic Production of Relativistic Jets |
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