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Max-Planck-Institut für extraterrestrische Physik

 

Verweis Deutsche Version .  MPE . HEG  . X-Ray Astronomy . Wave . ROSAT . Gallery . ROSAT Calendar Images . 1995
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Spiral Galaxy NGC 4258

The ROSAT observation of the spiral galaxy NGC 4258, which exhibits "anomalous arms" and a Seyfert nucleus. In the upper left part of the figure the X-ray emission (contour lines) is superposed on a deep optical image. In the upper right part of the figure contour lines of the radio emission, which trace the anomalous arms, are superposed on a map of the hard X-ray emission. The lower parts of the figure show superpositions of the optical emission from the central region of the galaxy with the soft (left) and the hard (right) X-ray emission.

gzipped 300 dpi tif version


ROSAT (Röntgensatellit) 1995
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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