Emissionsliniengebiete in den Zentralgalaxien von Cooling-Flow Galaxienhaufen.

Mathematics

Scientific paper

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Scientific paper

Emissionsliniengebiete in den zentralen Galaxien von 3 Galaxienhaufen (A
1795, PKS 0745-191, 2A 0335+096), die aufgrund von
Röntgenbeobachtungen einen besonders massiven Cooling-Flow zeigen
sollten, wurden im Optischen spektroskopisch untersucht.

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