NGC 4410a/b: A strong radio source associated with interacting galaxies

Details NGC 4410a/b: A strong radio source associated with interacting galaxies NGC 4410a/b: A strong radio source associated with interacting galaxies

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155..161h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 1, Jan. 1986, p. 161-168.

Astronomy and Astrophysics

Astronomy

13

Galaxies, Interacting Galaxies, Radio Sources (Astronomy), Tides, Astronomical Maps, Astronomical Photography, Celestial Mechanics, High Resolution, Radial Velocity, Radiant Flux Density, Very Large Array (Vla)

Scientific paper

The tidally interacting pair of galaxies NGC 4410a/b is in a group of galaxies. Two members of the group form with NGC 4410 a chain linked by bridges of diffuse, but knotty, optical emission. The radio source associated with NGC 4410 is studied in detail with the aid of observations done with the Very Large Array. The source has a radio luminosity (L ≅ 7×1040erg s-1) comparable to low luminosity radio galaxies and is very asymmetric with respect to NGC 4410. Its size is much larger than the optical size of NGC 4410. Some features, if not all, of the radio source are probably related to the interaction.

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