The central region of NGC 613. Evidence for an accelerated collimated outflow

Details The central region of NGC 613. Evidence for an accelerated collimated outflow The central region of NGC 613. Evidence for an accelerated collimated outflow

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...172...51h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 172, no. 1-2, Jan. 1987, p. 51-54.

Astronomy and Astrophysics

Astronomy

30

Barred Galaxies, Collimation, Flow Velocity, Galactic Nuclei, Radio Jets (Astronomy), Astronomical Maps, Astronomical Spectroscopy, Line Spectra, Radial Velocity

Scientific paper

Observations performed with the VLA at 6 and 20 cm reveal a nuclear radio jet in the central region of the barred spiral galaxy NGC 613. CCD surface photometry in O III 5007 A forbidden line light shows a corresponding optical feature. Optical spectroscopy shows excess velocities in the O III forbidden line along this feature, which can be interpreted as outflow perpendicular to the plane of the galaxy. In addition, an extended radio structure surrounds the nucleus.

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