Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296.1065t&link_type=abstract
In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background p 1065-1067 (SEE N90-2
Astronomy and Astrophysics
Astronomy
Brightness Distribution, Galactic Clusters, Galactic Radiation, X Ray Spectra, Emission Spectra, Galactic Structure, Star Clusters, Stellar Luminosity
Scientific paper
The absolute surface brightness around the Coma-A1367 supercluster region is measured on board Ginga. Data obtained by the scanning observation was analyzed and discrete sources of down to 0.2 mCrab were selected. For the residual sky without resolved sources, the surface brightness distribution was analyzed. The data is compared with the fluctuation caused by the emission from unresolved discrete sources assuming the previously known log N-log S relation. The result shows that these distributions are consistent with each other, showing that there is no clear excess structure in the X-ray surface brightness of Coma-A1367 supercluster region.
Awaki Hisamitsu
Kawada Mitsunobu
Koyama Katsuji
Takano Shiro
Tawara Yuzura
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