Using the European X-ray astronomy satellite XMM-Newton(1), researchers from CNRS(2) and CEA (3) 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(4) 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-Newton 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 cosmic rays(5) has been discovered outside the Solar System. It shows that the shock waves 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 particles on star formation.
Notes:
(1) XMM-Newton is an ESA satellite to which CNES, CEA and CNRS have made a significant contribution.
(2) Laboratories involved: Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse (CNRS/Universite Paris-Sud), Laboratoire d’Annecy le Vieux de Physique des Particules (CNRS/Universite de Savoie), Laboratoire Astrophysique, Interactions, Multi-echelles (CEA/CNRS/Universite Paris-Diderot).
(3) Institut de Recherches sur les Lois Fondamentales de l’Univers (Irfu), Service d’astrophysique.
(4) Cosmic rays whose kinetic energy is less than half a billion electronvolts.
(5) The cosmic rays discovered are hadronic, in other words largely made up of atomic nuclei. Hadronic cosmic rays make up about 99% of the galactic particles detected in the vicinity of the Earth. Electrons and positrons, which make up the leptonic component of cosmic rays, are far less abundant.
References:
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,
View web site – http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201219016&Itemid=129
Contact information:
Researchers:
Vincent Tatischeff, Tel 01 69 15 52 41, vincent.tatischeff@csnsm.in2p3.fr
Anne Decourchelle, Tel 01 69 08 43 84, anne.decourchelle@cea.fr
Gilles Maurin,Tel 04 50 09 16 75, gilles.maurin@lapp.in2p3.fr
CNRS Press Office:
Julien Guillaume, Tel 01 44 96 51 51, julien.guillaume@cnrs-dir.fr
