Electromagnetic jets from compact objects
Description
The possibility that at least some astrophysical jets are initially electromagnetic in origin is examined. Subsequent pick-up of ionization would convert such electromagnetic jets into hydrodynamic jets. In such a model, relativistic outflow is formed into highly collimated beams simply through the interaction with the surrounding medium. Forming jets under such general circumstances is encouraging in view of the range of scales that appear to be involved. The overall properties of such jets are largely determined by a single dimensionless parameter: the characteristic electrostatic potential drop rewritten as a particle Lorentz factor. Consequently, the determination of any one observable, such as the total power output, also determines the particle energy scale, the electromagnetic field strengths, etc. 18 references
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 321
- Series
- Astrophys. J.
- Journal Page Range
- 714-720
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19043164
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHARGED PARTICLES; COSMIC RADIO SOURCES; ELECTRIC FIELDS; ELECTROMAGNETIC RADIATION; GALAXY NUCLEI; HYDRODYNAMICS; LORENTZ FORCE; ORIGIN; PLASMA JETS
- Descriptors DEC
- FLUID MECHANICS; MECHANICS; RADIATIONS