New type of cosmic ray discovered after 100 years

October 16, 2012, CNRS
The region of the Arches cluster seen in X-rays (contours) and in the near infrared (background image). The infrared map is obtained from observations by the Hubble space telescope at the 1.875 µm wavelength (data taken from Dong et al. 2011, Monthly Notices of the Royal Astronomical Society, 417, 114). The contours show the strength of the neutral iron line observed by XMM-Newton around the star cluster (located in the center of the image). The X-ray emission is produced by cosmic rays accelerated in the shock wave formed in the interstellar medium by the supersonic motion of the cluster. In the image, the cluster is traveling from right to left at about 700 000 km/h. Credit: V. Tatischeff.

(—Using the European X-ray astronomy satellite XMM-Newton, researchers from CNRS and CEA have discovered a new source of cosmic rays. In the vicinity of the remarkable Arches cluster, near the center of the Milky Way, these particles are accelerated in the shock wave generated by tens of thousands of young stars moving at a speed of around 700,000 km/h. These cosmic rays produce a characteristic X-ray emission by interacting with the atoms in the surrounding gas. Their origin differs from that of the cosmic rays discovered exactly a hundred years ago by Victor Hess, which originate in the explosions of supernovae. The findings are published in the journal Astronomy & Astrophysics.

A hundred years ago, the Austrian physicist Victor Franz Hess discovered the existence of ionizing radiation of extraterrestrial origin, which he called cosmic rays. Today, their nature is well understood. When certain stars at the end of their lives explode and become supernovae, their matter is ejected at supersonic speed, generating shock waves that accelerate the particles. As a result, some atomic nuclei gain very high kinetic energy and enter the Earth's atmosphere.

However, low-energy cosmic rays are not detected in the region of our planet, since the solar wind prevents them from entering the heliosphere. Little is therefore known about their chemical composition and flux outside the Solar System, although everything suggests they play a significant role in the Galaxy. For instance, by ionizing and heating the densest interstellar clouds, they probably regulate the formation of stars.

The authors of the article began by studying the X-ray emission that should theoretically be generated by low-energy cosmic rays in the interstellar medium. They then looked for signs of this theoretical emission in X-ray data collected by XMM- since its launch in 1999. By analyzing the properties of the X-ray emission of interstellar iron recorded by the satellite, they found the signatures of a large fast ion population in the vicinity of the Arches cluster, about one hundred light-years from the center of the Milky Way. The stars in this cluster are traveling together at a speed of approximately 700,000 km/h. The cosmic rays are in all likelihood produced in the high-speed collision of the star cluster with a gas cloud in its path. In this particular region, the energy density of the accelerated ions is around a thousand times greater than that of cosmic rays in the neighborhood of the Solar System.  

This is the first time that a major source of low-energy has been discovered outside the Solar System. It shows that the of supernovae are not the only objects that can cause mass acceleration of atomic nuclei in the Galaxy. These findings should make it possible to identify new sources of ions in the interstellar medium, and may lead to a better understanding of the effects of these energetic on star formation.  

Explore further: Galactic Center Found To Glow Unevenly

More information: Nonthermal X-rays from low-energy cosmic rays: Application to the 6.4 keV line emission from the Arches cluster region, V. Tatischeff, A. Decourchelle, and G. Maurin, A&A, 2012, 546, A88,

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4.7 / 5 (14) Oct 16, 2012
All right, maybe I'm just in nitpicking mode today, but when I saw this article I thought "Really!?!" Wouldn't this article be more aptly named "New source of cosmic rays..." instead of "New type..."?
4 / 5 (4) Oct 16, 2012
I agree with you PhotonX... but it's not like Physorg hasn't used sensational headlines before.

The stars in this cluster are traveling together at a speed of approximately 700,000 km/h.

Relative to what? Why do they just state a meaningless velocity... shoddy work folks.
1 / 5 (6) Oct 17, 2012
Nonthermal x-rays ... What have I been saying all along. It doesn't take millions of degrees to create x-rays. The solar corona is an example of the very thing they are discussing here. Solar particles(cosmic rays) disturbing the surrounding gases. It won't be long till people will read my theories and say "duh..anybody can see that. What's the big deal?"
2.3 / 5 (3) Oct 17, 2012
100% of these comments should be deleted.
3 / 5 (4) Oct 17, 2012
Ok, I fell for it. I took 30 seconds to look up D.T. Yarbrough to see what his "theories" are. 30 seconds of my life wasted, that I will never get back.
5 / 5 (2) Oct 17, 2012
I agree with you PhotonX... but it's not like Physorg hasn't used sensational headlines before.

Physorg doesn't author anything. This is an aggregation site. All the headlines (and the content of all the articles) are verbatim copies from the source (that's why you sometimes see weird line-breaks and hyphenations here. Because the paragraph width may differ from the source).

Just paste the headline into google. You'll see what I mean.
not rated yet Oct 17, 2012
Aren't Bob, Lisa, et al. Physorg staff writers? Or are least as regular contributors they come pretty close.
5 / 5 (3) Oct 17, 2012
If you go to the 'about' section it says they have 7 (full time) staff and 6 (presumably non-full time) writers. Physorg adds 75 to 100 articles per day (as per the wikipedia entry on physorg) - even on weekends and around the clock. So by my count that means at any one time you have max. 3-4 people actively looking after the site and working on it.

Researching and properly writing up an article takes a bit of time (as does administration work). So the overwhelming part is likely aggregated from other sources.

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