Detection of the High-Energy Cosmic Rays from the Monogem Ring

, , and

Published 2003 October 21 © 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation A. Chilingarian et al 2003 ApJ 597 L129 DOI 10.1086/380190

1538-4357/597/2/L129

Abstract

The MAKET-ANI detector reveals significant excess of extensive air showers with arrival directions pointed to the Monogem ring, a supernova remnant located at a distance of ≈300 pc from the Sun with ≈100 kyr old radio pulsar PSR B0656+14 near the center. The chances that this excess is due to the fluctuations of an isotropic flux is 2 per million. For the search of the cosmic-ray source, we use the MAKET-ANI detector data from years 1997 to 2003. The best signal bin coordinates, right ascension 7fh5, declination 14° (750+14), significantly deviate from the ring morphological center, shifted in the direction of the most intensive X-ray emission from the supernova remnant's limb, now located 66 pc from the supernova remnant center and 27 pc from the candidate source.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/380190