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Astronomers reveal a cosmic "Axis of Evil"

Measurements used to weigh galaxy clusters carried out in three different wavelengths are giving rise to significantly different results.
Astronomers are puzzled by the announcement that the masses of the largest objects in the universe appear to depend on which method is used to weigh them. The new work was presented at a specialist discussion meeting on “Scaling Relations of Galaxy Clusters” organized by the Astrophysics Research Institute (ARI) at Liverpool John Moores University and supported by the Royal Astronomical Society.

Clusters of galaxies are the largest gravitationally bound objects in the universe, containing thousands of galaxies like the Milky Way, and their weight is an important probe of their dark matter content and evolution through cosmic time. Measurements used to weigh these systems carried out in three different regions of the electromagnetic spectrum — X-ray, optical, and millimeter wavelengths — give rise to significantly different results.

Eduardo Rozo from the University of Chicago explained that any two of the measurements can be made to fit easily enough but that always leaves the estimate using the third technique out of line. Dubbed the “Axis of Evil,” it is as if the universe is being difficult by keeping back one or two pieces of the jigsaw and deliberately preventing researchers from calibrating our weighing scales properly.

More than 40 of the leading cluster astronomers from the United Kingdom, Europe, and the United States attended the meeting to discuss the early results from the Planck satellite, currently scanning the heavens at millimeter wavelengths, looking for the smallest signals from clusters of galaxies and the cosmic background radiation in order to understand the birth of the universe. The Planck measurements were compared with optical images of clusters from the Sloan Digitized Sky Survey and new X-ray observations from the XMM-Newton satellite.

ARI astronomers are taking a leading role in this research through participation in the X-ray cluster work and observations of the constituent galaxies using the largest ground-based optical telescopes.

One possible resolution to the “Axis of Evil” problem discussed at the meeting is a new population of clusters that is optically bright but also X-ray faint. Jim Bartlett from the University of Paris, who is one of the astronomers who presented the Planck results, argued that the prospect of a new cluster population that responds differently was a “frightening prospect” because it overturns age-old ideas about the gravitational physics being the same from cluster to cluster.

“I saw this meeting as an opportunity to bring together experts who study clusters at only one wavelength and don’t always talk to their colleagues working at other wavelengths,” said Chris Collins from ARI. “The results presented are unexpected, and all three communities — optical, X-ray, and millimeter — will need to work together in the future to figure out what is going on.”

Coma-cluster
The Coma Cluster is a massive cluster of galaxies in the local universe. NASA/ESA/and the Hubble Heritage Team (STScI/AURA). Acknowledgment: D. Carter (Liverpool John Moores University) and the Coma HST ACS Treasury Team
Astronomers are puzzled by the announcement that the masses of the largest objects in the universe appear to depend on which method is used to weigh them. The new work was presented at a specialist discussion meeting on “Scaling Relations of Galaxy Clusters” organized by the Astrophysics Research Institute (ARI) at Liverpool John Moores University and supported by the Royal Astronomical Society.

Clusters of galaxies are the largest gravitationally bound objects in the universe, containing thousands of galaxies like the Milky Way, and their weight is an important probe of their dark matter content and evolution through cosmic time. Measurements used to weigh these systems carried out in three different regions of the electromagnetic spectrum — X-ray, optical, and millimeter wavelengths — give rise to significantly different results.

Eduardo Rozo from the University of Chicago explained that any two of the measurements can be made to fit easily enough but that always leaves the estimate using the third technique out of line. Dubbed the “Axis of Evil,” it is as if the universe is being difficult by keeping back one or two pieces of the jigsaw and deliberately preventing researchers from calibrating our weighing scales properly.

More than 40 of the leading cluster astronomers from the United Kingdom, Europe, and the United States attended the meeting to discuss the early results from the Planck satellite, currently scanning the heavens at millimeter wavelengths, looking for the smallest signals from clusters of galaxies and the cosmic background radiation in order to understand the birth of the universe. The Planck measurements were compared with optical images of clusters from the Sloan Digitized Sky Survey and new X-ray observations from the XMM-Newton satellite.

ARI astronomers are taking a leading role in this research through participation in the X-ray cluster work and observations of the constituent galaxies using the largest ground-based optical telescopes.

One possible resolution to the “Axis of Evil” problem discussed at the meeting is a new population of clusters that is optically bright but also X-ray faint. Jim Bartlett from the University of Paris, who is one of the astronomers who presented the Planck results, argued that the prospect of a new cluster population that responds differently was a “frightening prospect” because it overturns age-old ideas about the gravitational physics being the same from cluster to cluster.

“I saw this meeting as an opportunity to bring together experts who study clusters at only one wavelength and don’t always talk to their colleagues working at other wavelengths,” said Chris Collins from ARI. “The results presented are unexpected, and all three communities — optical, X-ray, and millimeter — will need to work together in the future to figure out what is going on.”

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