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.

Crédito:

ESO

Sobre la imagen

Identificador:eso0221e
Tipo:Observación
Fecha de publicación:7 de Agosto de 2002
Noticias relacionadas:eso0221
Tamaño:723 x 955 px

Sobre el objeto

Nombre:CL0053-37
Tipo:Early Universe : Cosmology : Phenomenon : Dark Matter
Early Universe : Galaxy : Grouping : Cluster
Distancia:z=0.162 (desplazamiento al rojo)
Categoría:Galaxy Clusters

Formatos de imagen

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732,6 KB
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Colores y filtros

BandaTelescopio
ÓpticoMPG/ESO 2.2-metre telescope
WFI

Notas: .