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.

Kredit:

ESO

O snímku

Id:eso0221e
Typ:Pozorování
Datum zveřejnění:7. srpna 2002
Související články:eso0221
Velikost:723 x 955 px

O objektu

Jméno:CL0053-37
Typ:Early Universe : Cosmology : Phenomenon : Dark Matter
Early Universe : Galaxy : Grouping : Cluster
Vzdálenost:z=0.162 (rudý posuv)
Kategorie:Galaxy Clusters

Image Formats

největší JPEG
233,1 KB

Pozadí

1024x768
228,0 KB
1280x1024
309,9 KB
1600x1200
381,5 KB
1920x1200
364,2 KB
2048x1536
504,5 KB

Barvy & filtry

PásmoDalekohled
OptickýMPG/ESO 2.2-metre telescope
WFI

Poznámky: .