PROGRAM: SL-1

AYS FROM A KYOTO MILLENNIUM SUPERNOVA REMNANT (SNR)
K Koyama*
*Department of Physics, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto, 606-8502, Japan

Abstract:

This paper reports on the Origin of the Galactic Cosmic Rays, the abundances of heavy elements and asymmetric distribution of the heavy elements in the ejecta of the supernova remnants. The data are taken with the ASCA and Suzaku satellite in a historical type I a supernova SN1006 (Koyama et al, 1995, Uchida et al 2013, Yamaguchi et al. 2008). The results are compared with the historical reports in AD 1230 in the diary of Meigetsuki, a national treasure of Japan (Fujiwara, T. 1232). The results demonstrate that the old historical record gives very important implications on the modern astronomy. This paper reports the details on these issues.

Acknowledgements:

The author express his sincere thanks to all the members of the ASCA and Suzaku satellites, the fourth and fifth X-ray satellite of Japan.

References:

Fujiwara, T, Meigetsuki, Vol 48 120
Koyama, K et al. Nature 1995, 378, 255
Uchida, H., Yamaguchi, H. & Koyama, K. 2013, ApJ, 771, 56
Yamaguchi et al. 2008, PASJ, 60, 141

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