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Title:
A model for elliptical radio galaxies with dust lanes
Authors:
van Albada, T. S.; Kotanyi, C. G.; Schwarzschild, M.
Affiliation:
AA(Groningen, Rijksuniversiteit, Groningen, Netherlands), AB(Groningen, Rijksuniversiteit, Groningen, Netherlands)
Publication:
Royal Astronomical Society, Monthly Notices, vol. 198, Jan. 1982, p. 303-310. Research supported by the Nederlandse Organisatie voor Zuiver-Wetenschappelijk Onderzoek (MNRAS Homepage)
Publication Date:
01/1982
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
ASTRONOMICAL MODELS, COSMIC DUST, ELLIPTICAL GALAXIES, GAS DYNAMICS, RADIO GALAXIES, ASTRONOMICAL MAPS, ASTRONOMICAL PHOTOGRAPHY, GALACTIC STRUCTURE, ORBIT CALCULATION, STELLAR SYSTEMS
Comment:
A&AA ID. AAA031.151.001
Bibliographic Code:
1982MNRAS.198..303V

Abstract

The stationary states of motion of gas in a triaxial stellar system which rotates about one of its principal axes are described. It is noted that four dynamically different situations are possible and that in two of these the gas layer is warped. The morphology of elliptical radio galaxies with dust lanes, such as NGC 5128 (Cen A) and M84, can be understood through this model; transient phenomena are not required.

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