Rotation of the dust lane in NGC 1947

Details Rotation of the dust lane in NGC 1947 Rotation of the dust lane in NGC 1947

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..130m&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 1, Apr. 1982, p. 130-133.

Astronomy and Astrophysics

Astrophysics

22

Cosmic Dust, Elliptical Galaxies, Galactic Rotation, Interstellar Gas, Image Tubes, Radial Velocity, Radio Galaxies

Scientific paper

Long slit image tube spectrograms of the southern dust lane galaxy NGC
1947 were obtained in order to study the kinematics of this
object. The dust lane shows fast rotation while the stellar component
does (nearly) not rotate. The system shows strong similarity to NGC
5128 (Cen A), however is not a radio galaxy.

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