31 Mar

File:Rosat 0.75kev diffuse background map.gif

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Revision as of 12:52, 31 March 2013
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The 3/4 keV band map from the ROSAT survey. Note how different the structure is from the 1/4 keV band map. The 3/4 keV data are relatively flat across the sky with the addition of distinct Galactic features. The largest is Loop I, the ~100 degree ring of enhanced emission in the Galactic center direction. This is thought to be a supernova remnant/stellar wind bubble at a distance of 150 parsecs and a radius of ~100 parsecs.

The 3/4 keV band map from the ROSAT survey. Note how different the structure is from the 1/4 keV band map. The 3/4 keV data are relatively flat across the sky with the addition of distinct Galactic features. The largest is Loop I, the ~100 degree ring of enhanced emission in the Galactic center direction. This is thought to be a supernova remnant/stellar wind bubble at a distance of 150 parsecs and a radius of ~100 parsecs.
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== {{int:license}} ==
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== {{int:license-header}} ==

{{PD-USGov-NASA}}

{{PD-USGov-NASA}}

[[Category:ROSAT]]

[[Category:ROSAT]]
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[[Category:Aitoff allsky views]]
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[[Category:Astronomical maps]]

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[[Category:Maps with Hammer projection]]

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