An X-ray study of A2199 and A2197.

Details An X-ray study of A2199 and A2197. An X-ray study of A2199 and A2197.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..601m&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 601 - 602

Astronomy and Astrophysics

Astrophysics

2

Clusters Of Galaxies: X Rays, Clusters Of Galaxies: Morphology, Clusters Of Galaxies: Intracluster Gas, Clusters Of Galaxies: Temperatures, Clusters Of Galaxies: Surface Brightness, Clusters Of Galaxies: Luminosities, Clusters Of Galaxies: Masses, Clusters Of Galaxies: Cooling

Scientific paper

In this work the authors analyse the X-ray properties of the clusters of galaxies Abell 2199 and Abell 2197. Particular emphasis is put on the search for evidence of a physical relation between both clusters. In an area of 4°×4° around the pair of clusters the authors search for X-ray emissions assuming the possible existence of hot gas associated with the Hercules supercluster. For both clusters they determine the surface brightness, intra-cluster gas temperature, luminosity, mass, central cooling time and morphological properties. The X-ray data consist in ROSAT PSPC pointed observations and ROSAT All-Sky Survey data. The authors also compare the X-ray morphology with two different galaxy distributions: galaxies coming from the APM catalog and the sample selected by Gregory and Thompson (1984).

Affiliated with

Also associated with

No associations

Rating

An X-ray study of A2199 and A2197. 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 An X-ray study of A2199 and A2197., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An X-ray study of A2199 and A2197. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-858262