Optical and X-ray view of the Helix Nebula | ||||
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Minimum credit line: Image courtesy of Marco Iacobelli (XMM-Newton SOC) and ESA. (for details, see Conditions of Use). Credit: ESA/XMM-Newton, CC BY-SA 3.0 IGO The image above can be displayed at full size and may be downloaded by clicking the image above. |
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This composite optical (DSS) and X-ray (XMM-Newton EPIC) view depicts the Helix Nebula (also known as The Helix or NGC 7293), a large planetary nebula and one of the closest to the Earth at a distance of about 700 light-years. The central stellar core remnant, known as planetary nebula nucleus, is a compact star (the X-ray bright source clearly visible at the center of the nebula); gases from the outer layers of the star ejected in the surrounding space are heated by the hot core of the dead star, and shine in different wavelenght bands ranging from the infrared to the optical. X-ray emission is colour coded as: red=0.3-1 keV, green=1-2 keV, blue=2-8 keV. Several point-like sources with different spectral properties fill the field of view.
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