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Perseus Cluster: Mysterious X-ray Signal Intrigues Astronomers
Visual Description:

  • A mysterious signal has been seen in X-ray data from a study of over 70 galaxy clusters with Chandra and XMM-Newton.

  • This spike of intensity at a specific wavelength of X-ray light has several intriguing explanations.

  • More data and investigation will be needed to confirm both the signal's existence and nature.

  • This image shows a new view of the Perseus cluster, one of the galaxy clusters included in the new study.

A new study of the central region of the Perseus galaxy cluster, shown in this image, using NASA's Chandra X-ray Observatory and 73 other clusters with ESA's XMM-Newton has revealed a mysterious X-ray signal in the data. This signal is represented in the circled data points in the inset, which is a plot of X-ray intensity as a function of X-ray energy. The signal is also seen in over 70 other galaxy clusters using XMM-Newton. This unidentified X-ray emission line - that is, a spike of intensity at a very specific energy, in this case centered on about 3.56 kiloelectron volts (keV) - requires further investigation to confirm both the signal's existence and nature as described in the latest Chandra press release.

One intriguing possible explanation of this X-ray emission line is that it is produced by the decay of sterile neutrinos, a type of particle that has been proposed as a candidate for dark matter. While holding exciting potential, these results must be confirmed with additional data to rule out other explanations and determine whether it is plausible that dark matter has been observed.

There is uncertainty in these results, in part, because the detection of this emission line is pushing the capabilities of both Chandra and XMM-Newton in terms of sensitivity. Also, there may be explanations other than sterile neutrinos if this X-ray emission line is deemed to be real. For example, there are ways that normal matter in the cluster could have produced the line, although the team's analysis suggested that all of these would involve unlikely changes to our understanding of physical conditions in the galaxy cluster or the details of the atomic physics of extremely hot gases.

This image is Chandra's latest view of hot gas in the central region of the Perseus Cluster, where red, green, and blue show low, medium, and high-energy X-rays respectively. It combines data equivalent to more than 17 days worth of observing time taken over a decade with Chandra. The Perseus Cluster is one of the most massive objects in the Universe, and contains thousands of galaxies immersed in an enormous cloud of superheated gas. In Chandra's X-ray image, enormous bright loops, ripples, and jet-like streaks throughout the cluster can be seen. The dark blue filaments in the center are likely due to a galaxy that has been torn apart and is falling into NGC 1275 (a.k.a. Perseus A), the giant galaxy that lies at the center of the cluster. A different view of Perseus, shown below, combines data from Chandra in the inner regions of the cluster and XMM data in regions further out.

A paper describing the detection of this mysterious emission line was published in the July 1st issue of The Astrophysical Journal and a preprint is available online. The first author is Esra Bulbul of Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, MA, and NASA's Goddard Space Flight Center (GSFC) in Greenbelt, MD. The co-authors are Maxim Markevitch from GSFC, Adam Foster and Randall Smith from CfA, Michael Loewenstein from University of Maryland in College Park MD and GSFC, and Scott W. Randall from CfA.

Only a week after Bulbul et al. placed their paper on the arXiv, a different group, led by Alexey Boyarsky of Leiden University in the Netherlands, placed a paper on the arXiv reporting evidence for an emission line at the same energy in XMM-Newton observations of the galaxy M31 and the outskirts of the Perseus cluster. This strengthens the evidence that the emission line is real and not an instrumental artifact.

Visual Description:

A Chandra X-ray Observatory image of the Perseus galaxy cluster is displayed, which features a dark pink and brown color scheme. The structure of the Perseus Cluster appears as swirling clouds of gas and dust with a slight figure 8-shape at its core and a puff of dark blue filamentary material coming off of it, reminiscent of a fading tornado. An accumulation of over 400 hours of Chandra observations of the central regions of the Perseus galaxy cluster reveals evidence of the turmoil that has wracked the cluster for hundreds of millions of years. One of the most massive objects in the universe, the Perseus cluster contains thousands of galaxies immersed in a vast cloud of multimillion degree gas with the mass equivalent of trillions of suns. Enormous bright loops, ripples, and jet-like streaks are also apparent in the image. The small dark blue filaments to the right in the center of the image are likely due to a galaxy that has been torn apart and is falling into NGC 1275, a.k.a. Perseus A, the giant galaxy that lies at the center of the cluster. To the lower left is a plot in white and blue and reflects a study of the central region of the Perseus galaxy cluster that revealed a mysterious X-ray signal in the data. This signal is represented in circled data points in the inset, which is a plot of X-ray intensity as a function of X-ray energy. This unidentified X-ray emission line - that is, a spike of intensity at a very specific energy, in this case centered on about 3.56 kiloelectron volts - requires further investigation to confirm both the signal's existence and nature.

 

Fast Facts for Perseus Cluster:
Credit  X-ray: NASA/CXC/SAO/E.Bulbul, et al.
Release Date  June 24, 2014
Scale  Image is about 11 arcmin across (about 768,000 light years)
Category  Groups & Clusters of Galaxies, Black Holes
Coordinates (J2000)  RA 03h 19m 47.60s | Dec +41° 30´ 37"
Constellation  Perseus
Observation Date  25 pointings between Sep 1999 and Dec 2009
Observation Time  416 hours 32 min (17 days 8 hours 32 min).
Obs. ID  502, 503, 1513, 3209, 3404, 4289, 4946-4953, 6139, 6145, 6146, 11713-11716, 12025, 12033, 12036, 12037
Instrument  ACIS
Also Known As Abell 426
References Bulbul, E. et al, 2014, ApJ (accepted); arXiv:1402.2301
Color Code  X-ray (Red = 0.5-1.2 keV, Green = 1.2-2.0 keV, Blue = 2.0-7.0 keV)
X-ray
Distance Estimate  About 250 million light years
distance arrow
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