Dark matter in CL 0053-37

A "map" of the dark matter distribution (black contours) in the cluster of galaxies CL0053-37, as obtained from the weak lensing effects detected in the WFI images, and the X-ray flux (green contours) taken from the All-Sky Survey carried out by the ROSAT satellite observatory. The distribution of galaxies resembles the elongated, dark-matter profile. Because of ROSAT's limited image sharpness (low "angular resolution"), it cannot be entirely ruled out that the observed X-ray emission is due to an active nucleus of a galaxy in CL0053-37, or even a foreground stellar binary system in NGC 300.

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ESO

Om bilden

ID:eso0221e
Typ:Observation
Publiceringsdatum:7 augusti 2002
Relaterade pressmeddelanden:eso0221
Storlek:723 x 955 px

Om objektet

Namn:CL0053-37
Typ:Early Universe : Cosmology : Phenomenon : Dark Matter
Early Universe : Galaxy : Grouping : Cluster
Avstånd:z=0.162 (rödförskjutning)
Kategori:Galaxy Clusters

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Originalstorlek
732,6 kB
Stor jpeg
233,1 kB
Skärmstor jpeg
289,6 kB

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Färger och filter

BandTeleskop
Synligt ljusMPG/ESO 2.2-metre telescope
WFI

Noter: .