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Verweis Deutsche Version .  MPE . HEG  . X-Ray Astronomy . Wave . ROSAT . Gallery . ROSAT Calendar Images . 1996
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Supernova Remnant G 272.2-3.2

The supernova remnant G 272.2-3.2 was discovered in 1990 during the ROSAT All-Sky Survey. It attracted attention by its relative hard X-ray emission pointing to temperatures between 7 and 10 million degrees, so that this object is relatively young (about 2000 years). The image was extracted from a six hour observation. The overlayed optical exposure shows a filament which was formed during the collision of the shock wave with an interstellar cloud.

gzipped high-resolution tif image


ROSAT (Röntgensatellit) 1996
Images from the X-ray sky with the ROSAT telescope · All rights reserved:
© Max-Planck-Institut für extraterrestrische Physik, Postfach 1603, 85740 Garching, Germany.
The X-ray images are produced by the SASS/EXSAS software MPE, ESO-MIDAS.
The ROSAT project is managed by the Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany on behalf of the Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie (BMBF).


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