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Chandra X-ray Observatory image of Abell 1795 galaxy cluster showcasing a cooling flow. Brighter areas indicate higher X-ray intensity, revealing gas condensing and cooling, potentially forming future stars.  A large galaxy at the top appears to have created a wake in the cluster's gas.

Chandra X-ray Observatory image of Abell 1795 galaxy cluster showcasing a cooling flow. Brighter areas indicate higher X-ray intensity, revealing gas condensing and cooling, potentially forming future stars. A large galaxy at the top appears to have created a wake in the cluster's gas.

Astronomy Picture from 08/12/2000

Abell 1795: A Galaxy Cluster's Cooling Flow

Source: https://apod.nasa.gov/apod/ap001208.html


#GalaxyClusters #ChandraXray #CoolingFlow #Abell1795 #SpaceScience #Astrophysics #XrayAstronomy #Cosmology #GalaxyFormation #DeepSpace

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H$α$-X-ray Surface Brightness Correlation for Filaments in Cooling Flow Clusters Massive galaxies in cooling flow clusters display clear evidence of feedback from Active Galactic Nuclei (AGN). Joint X-ray and radio observations have shown that AGN radio jets push aside the surroun...

Hα-X-ray Surface Brightness Correlation for Filaments in #CoolingFlow Clusters: arxiv.org/abs/2501.01902 -> Black Holes Can Cook for Themselves, Chandra Study Shows: chandra.cfa.harvard.edu/photo/2025/f...

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