The short wide angle tail radio source in NGC4874

Details The short wide angle tail radio source in NGC4874 The short wide angle tail radio source in NGC4874

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...147l..13f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 147, no. 1, June 1985, p. L13-L15.

Astronomy and Astrophysics

Astronomy

19

Astronomical Maps, Galactic Clusters, Galactic Radio Waves, Radio Sources (Astronomy), Galactic Structure, Interstellar Matter

Scientific paper

Radio maps at 1.5 and 4.9 GHz are presented of the radio source associated with NGC 4874, one of the two dominant galaxies of the Coma cluster. This radio source of the WAT type, has a very small linear size and is all contained within the optical galaxy. The existence of a very short WAT source implies that either the role of interstellar medium in bending the radio structure is not negligible, or the transition between interstellar and intergalactic medium occurs very close to the center of the galaxy, or other mechanisms are responsible for the wide angle tail phenomenon.

Affiliated with

Also associated with

No associations

Rating

The short wide angle tail radio source in NGC4874 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 The short wide angle tail radio source in NGC4874, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The short wide angle tail radio source in NGC4874 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1663230