An Hα–X-ray Surface-Brightness Correlation for Filaments in Cooling-Flow Clusters
Study on the Hα-X-ray Surface Brightness Correlation of Filamentary Structures in Cooling-Flow Clusters Background Introduction In the large-scale structure of the universe, cooling-flow clusters are a crucial type of celestial system. The cores of these galaxy clusters are typically dominated by massive galaxies (brightest cluster galaxies, BCGs) ...