k Perseus galaxy cluster, satellite image Perseus galaxy cluster, satellite image. The Perseus cluster Abell 426 is a cluster of galaxies in the constellation Perseus. A new study of the Perseus galaxy cluster and others using Chandra and XMMNewton has revealed a mysterious Xray signal in the data. The signal is also seen in over 70 other galaxy clusters using XMMNewton. This unidentified Xray emission line a spike of intensity centred on about 3.56 kiloelectron volts requires further investigation to confirm both the signals existence and nature. One possibility is this signal is from the decay of sterile neutrinos, one proposed candidate to explain dark matter. Imaged by the ESAs European Space Agencys XMMNewton space observatory. Photo by Chandra NASACXCSAOE.Bulbul, et al. XMMNewton ESASCIENCE PHOTO LIBRARY Stock Photo - Afloimages
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Perseus galaxy cluster, satellite image Perseus galaxy cluster, satellite image. The Perseus cluster  Abell 426  is a cluster of galaxies in the constellation Perseus. A new study of the Perseus galaxy cluster and others using Chandra and XMM Newton has revealed a mysterious X ray signal in the data. The signal is also seen in over 70 other galaxy clusters using XMM Newton. This unidentified X ray emission line   a spike of intensity centred on about 3.56 kiloelectron volts   requires further investigation to confirm both the signal s existence and nature. One possibility is this signal is from the decay of sterile neutrinos, one proposed candidate to explain dark matter. Imaged by the ESA s  European Space Agency s  XMM Newton space observatory. Photo by Chandra: NASA CXC SAO E.Bulbul, et al.  XMM Newton: ESA SCIENCE PHOTO LIBRARY
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Perseus galaxy cluster, satellite image

Perseus galaxy cluster, satellite image. The Perseus cluster (Abell 426) is a cluster of galaxies in the constellation Perseus. A new study of the Perseus galaxy cluster and others using Chandra and XMM-Newton has revealed a mysterious X-ray signal in the data. The signal is also seen in over 70 other galaxy clusters using XMM-Newton. This unidentified X-ray emission line - a spike of intensity centred on about 3.56 kiloelectron volts - requires further investigation to confirm both the signal's existence and nature. One possibility is this signal is from the decay of sterile neutrinos, one proposed candidate to explain dark matter. Imaged by the ESA's (European Space Agency's) XMM-Newton space observatory. Photo by Chandra: NASA/CXC/SAO/E.Bulbul, et al.; XMM-Newton: ESA/SCIENCE PHOTO LIBRARY

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