CXC Home | Search | Help | Image Use Policy | Latest Images | Privacy | Accessibility | Glossary | Q&A
1
A2142 - Optical Image
The two large elliptical galaxies indicated by arrows in the center of image are aligned in the general direction of the X-ray brightness elongation. They are thought to be the central galaxies of two sub-clusters that are participating in the merger.
(Credit: Palomar Digitized Sky Survey)
The two large elliptical galaxies indicated by arrows in the center of image are aligned in the general direction of the X-ray brightness elongation. They are thought to be the central galaxies of two sub-clusters that are participating in the merger.
(Credit: Palomar Digitized Sky Survey)
2
A2142 - Optical Image with X-ray
contours
The two large elliptical galaxies indicated by arrows in the center of image are aligned in the general direction of the X-ray brightness elongation. They are thought to be the central galaxies of two sub-clusters that are participating in the merger. The optical image is overlaid with X-ray brightness contours.
(Credit: Palomar Digitzed Sky Survey and NASA/CXC/SAO)
The two large elliptical galaxies indicated by arrows in the center of image are aligned in the general direction of the X-ray brightness elongation. They are thought to be the central galaxies of two sub-clusters that are participating in the merger. The optical image is overlaid with X-ray brightness contours.
(Credit: Palomar Digitzed Sky Survey and NASA/CXC/SAO)
4
Rosat Image of A2142
This image of A2142 was made the German Roentgensatellite (Rosat) X-ray observatory using the Position Sensitive Proportional Counter. It shows the entire cluster. The image is 30 arcminutes on a side.
(Credit: Rosat/J.P. Henry & U. Briel)
This image of A2142 was made the German Roentgensatellite (Rosat) X-ray observatory using the Position Sensitive Proportional Counter. It shows the entire cluster. The image is 30 arcminutes on a side.
(Credit: Rosat/J.P. Henry & U. Briel)
Return to A2142 Image (01 Mar 00)