High resolution radio and X-ray observations of A115

Details High resolution radio and X-ray observations of A115 High resolution radio and X-ray observations of A115

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...139...50f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 139, no. 1, Oct. 1984, p. 50-54.

Astronomy and Astrophysics

Astrophysics

21

Galactic Clusters, Galactic Structure, Radio Galaxies, X Ray Sources, Astronomical Maps, High Resolution, Interstellar Gas

Scientific paper

High resolution radio and X-ray observations are presented for the cluster of galaxies Abell 115, which is known in the literature for being characterized by a double X-ray structure and a multiple optical structure. The brightest galaxy of the cluster is associated with the radio source 3C28, which shows a very unusual radio morphology in the high resolution map presented here. A tail-type radio source is also found at about 4 arcmin from 3C28, in NE direction. A resolved X-ray structure is detected around 3C28, and is interpreted to originate from a hot gas which is likely to be accreting onto the galaxy. The complex radio structure of 3C28 is understood by invoking a combination of external ram pressure plus buoyancy effects of light radio plasmoids.

Affiliated with

Also associated with

No associations

Rating

High resolution radio and X-ray observations of A115 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 High resolution radio and X-ray observations of A115, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High resolution radio and X-ray observations of A115 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1226233