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ROSAT Guest Observer Facility

Images of the Cygnus Loop

This supernova remnant in the constellation Cygnus, known as the Cygnus Loop, is roughly 20,000 years old. It is generally circular in shape except for a break-out towards the south. In addition, there are many bright, filamentary structures. The ROSAT PSPC observation has allowed the temperature and density structure to be studied on a fine angular scale.

Cygnus Loop PSPC

(Credit: S. L. Snowden)

Figure a) of the PSPC plate shows the hard band (0.5-2.0 keV) mosaic of the Cygnus Loop and Figure b) shows the soft band (0.1 - 0.3 keV). (In all of these figures, purple and blue indicate low values while yellow and red indicate high values.) While the general structure in the two bands is reasonably similar, there are certain differences. This is easily seen in Figure c) which shows the hard/soft band ratio. In general, the interior of the Loop is harder and therefore hotter than the edge. This type of temperature gradient is consistent with what is expected. Figure d) shows the exposure time of the PSPC mosaic.
Get the high resolution (200 dpi) TIFF format version, or the high resolution Soft Band image.

Cygnus Loop HRI

(Credit: Levenson et al.)

The HRI image better shows the angular structure of the Cygnus Loop. Even with this image some of the fine-scale structure is not resolved (both because of the coarse angular binning and through insufficient event statistics).
Get the high resolution (200 dpi) TIFF format version.

Cygnus Loop Color HRI
Cygnus Loop HRI
(Credit: Levenson et al.)

A complete HRI image of the Cygnus Loop showing all the internal strucuture.
Get the high resolution (200 dpi) TIFF format version of the color image.
Get the high resolution (300 dpi) TIFF format version intensity image.

Curator: Michael Arida (SP Sys); arida@milkyway.gsfc.nasa.gov
HEASARC Guest Observer Facility
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This file was last modified on Friday, 25-Feb-2000 08:38:18 EST

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