Wind instability in the clouds around radio galaxies

Details Wind instability in the clouds around radio galaxies Wind instability in the clouds around radio galaxies

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..330v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, June 1982, p. 330-333.) Soviet Astronomy Letters, vol. 8, May-June 1982, p. 179, 180

Astronomy and Astrophysics

Astronomy

2

Intergalactic Media, Plasma Clouds, Radio Galaxies, Analogies, Astronomical Models, Earth Magnetosphere, Plasma Density

Scientific paper

In the magnetospheric model for the clouds around radio galaxies, wind instability should have a lower critical velocity than Kelvin-Helmholtz instability and a characteristic scale describing the most rapidly growing surface waves should be singled out. One thereby can evaluate the ratio of the cloud plasma density to the density in the circumfluent intergalactic medium.

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