Magneto gasdynamics of double radio sources

Details Magneto gasdynamics of double radio sources Magneto gasdynamics of double radio sources

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....79...40n&link_type=abstract

Astronomy and Astrophysics, vol. 79, no. 1-2, Oct. 1979, p. 40-47. Research supported by the Nederlandse Organisatie voor Zuive

Astronomy and Astrophysics

Astronomy

4

Intergalactic Media, Magnetohydrodynamic Flow, Plasma Clouds, Radio Sources (Astronomy), Magnetic Fields, Plasma Density, Radiation Distribution, Taylor Instability, Wakes

Scientific paper

Magnetogasdynamics of plasma clouds ejected into intergalactic matter is studied. A method of calculation is presented, along with initial conditions and assumptions that enable one to calculate radiation patterns. Results are described and discussed, and pertinent conclusions are drawn. It is found that low-density sources lose their coherence and are braked after 10-30 kpc, that high-density sources at high Mach number are not affected dynamically by magnetic fields, and that magnetic fields tend to lie along the ejection axis. Radiation patterns show that heads of clouds are always radiating regions, and wake radiation is also possible.

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