k Whirlpool galaxy, Xray image Whirlpool galaxy. Coloured Chandra Xray Telescope image of the Whirlpool galaxy M51, NGC 5194, showing sources which fall between the hard high energy, cosmic and soft low energy, galactic energies normally expected. These have been termed quasisoft sources and they lie in a temperature range of 1 to 4 million degrees Celsius. The Whirlpool galaxy is a spiral galaxy 13 million light years away in the constellation Canes Venatici. Xray sources of 0.31.0 keV are shown as red, 1.02.0 keV as green and 2.08.0 keV as blue. Taken over a period of 4 hours on June 20, 2000 with the Advanced CCD Imaging Spectrometer ACIS. Stock Photo - Afloimages
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Whirlpool galaxy, X ray image Whirlpool galaxy. Coloured Chandra X ray Telescope image of the Whirlpool galaxy  M51, NGC 5194 , showing sources which fall between the hard  high energy, cosmic  and soft  low energy, galactic  energies normally expected. These have been termed quasisoft sources and they lie in a temperature range of 1 to 4 million degrees Celsius. The Whirlpool galaxy is a spiral galaxy 13 million light years away in the constellation Canes Venatici. X ray sources of 0.3 1.0 keV are shown as red, 1.0 2.0 keV as green and 2.0 8.0 keV as blue. Taken over a period of 4 hours on June 20, 2000 with the Advanced CCD Imaging Spectrometer  ACIS .
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Whirlpool galaxy, X-ray image

Whirlpool galaxy. Coloured Chandra X-ray Telescope image of the Whirlpool galaxy (M51, NGC 5194), showing sources which fall between the hard (high energy, cosmic) and soft (low energy, galactic) energies normally expected. These have been termed quasisoft sources and they lie in a temperature range of 1 to 4 million degrees Celsius. The Whirlpool galaxy is a spiral galaxy 13 million light years away in the constellation Canes Venatici. X-ray sources of 0.3-1.0 keV are shown as red, 1.0-2.0 keV as green and 2.0-8.0 keV as blue. Taken over a period of 4 hours on June 20, 2000 with the Advanced CCD Imaging Spectrometer (ACIS).

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