The central velocity field of the Markaryan galaxy NGC 1614

Details The central velocity field of the Markaryan galaxy NGC 1614 The central velocity field of the Markaryan galaxy NGC 1614

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..389a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 389-392) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July-

Astronomy and Astrophysics

Astronomy

Emission Spectra, Galactic Nuclei, Galactic Rotation, Interstellar Gas, Radial Velocity, Galactic Structure

Scientific paper

Using spectrograms obtained on the diffraction spectrograph with image tube in the primary focus of the 6-m telescope the velocity field in the central region of the Mark 617 galaxy was investigated. Noncircular motions of gas found in the narrow interval of position angles of 70°-90° are explained by gas ejection from the nucleus along the small axis of the galaxy. A possible existence of large-scale radial motions of gas is noted.

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