Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795

Details Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795 Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.1313e&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #13.13; Bulletin of the American Astronomical Society, Vol. 32, p.1200

Astronomy and Astrophysics

Astronomy

Scientific paper

We present spatial and spectral analysis of the central 350 h50-1 kpc in radius of the cooling flow galaxy cluster A1795. A 30 arcsec filament extending to South of the cD galaxy appears in the X-ray map in coincidence with the Hα structure. The temperature of the plasma rises from about 2 keV in this region to about 5 keV at 3 arcmin from the X-ray centre. Two-dimensional distributions of the gas density, temperature, pressure, cooling time obtained from the spectral analysis are presented. Moreover, the constraints on the distribution of the dark matter in the cluster central region are discussed.

Affiliated with

Also associated with

No associations

Rating

Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795 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 Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra observation of the inner regions of the cooling-flow galaxy cluster A1795 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-870496