A ROSAT-HRI observation of the cluster MS0353-7411 (A3186).

Details A ROSAT-HRI observation of the cluster MS0353-7411 (A3186). A ROSAT-HRI observation of the cluster MS0353-7411 (A3186).

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..201n&link_type=abstract

Astrophysical Letters and Communications, Vol. 36, Nos. 1 - 6, p. 201 - 204

Astronomy and Astrophysics

Astrophysics

1

Clusters Of Galaxies: X Rays, Clusters Of Galaxies: Cooling Flows, Clusters Of Galaxies: Intergalactic Gas, Intracluster Gas: X-Ray Structure

Scientific paper

The X-ray emitting intracluster gas in the galaxy cluster Abell 3186 is
elongated in the SE - NW direction, while the galaxy isoplets are
basically N - S. Emission is peaked on the cD galaxy, but substantial
substructure exists. A small cooling flow (4 M˙sun/yr) is
found, although the cD galaxy has no emission lines.

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