A model for elliptical radio galaxies with dust lanes

Details A model for elliptical radio galaxies with dust lanes A model for elliptical radio galaxies with dust lanes

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..303v&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Jan. 1982, p. 303-310. Research supported by the Nederlandse Organ

Astronomy and Astrophysics

Astronomy

166

Astronomical Models, Cosmic Dust, Elliptical Galaxies, Gas Dynamics, Radio Galaxies, Astronomical Maps, Astronomical Photography, Galactic Structure, Orbit Calculation, Stellar Systems

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

A model for elliptical radio galaxies with dust lanes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A model for elliptical radio galaxies with dust lanes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A model for elliptical radio galaxies with dust lanes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1457628