Discovery of non-thermal X-rays from the northwest shell of the new SNR RX J1713.7-3946: The second SN 1006?

被引:246
作者
Koyama, K
Kinugasa, K
Matsuzaki, K
Nishiuchi, M
Sugizaki, M
Torii, K
Yamauchi, S
Aschenbach, B
机构
[1] OSAKA UNIV, FAC SCI, DEPT EARTH & SPACE SCI, TOYONAKA, OSAKA 560, JAPAN
[2] UNIV TOKYO, SCH SCI, DEPT PHYS, BUNKYO KU, TOKYO, JAPAN
[3] INST SPACE & ASTRONAUT SCI, SAGAMIHARA, KANAGAWA 229, JAPAN
[4] IWATE UNIV, FAC HUMANITIES & SOCIAL SCI, MORIOKA, IWATE 020, JAPAN
[5] JAPAN SCI & TECHNOL CORP, CREST, KAWAGUCHI, SAITAMA 332, JAPAN
[6] MAX PLANCK INST EXTRATERR PHYS, D-85740 GARCHING, GERMANY
关键词
interstellar; individual (RX J1713.7-3946); radiation mechanism; supernova remnants; X-rays; sources; spectra;
D O I
10.1093/pasj/49.3.L7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the ASCA results of a featureless X-ray spectrum from RX J1713.7-3946, a new shell-like SNR discovered with the ROSAT all-sky survey. The northwest part of RX J1713.7-3946 was in the field of the ASCA Galactic Plane Survey Project, and was found to exhibit a shell-like structure. The spectrum, however, shows neither line emission nor any signature of a thermal origin. Instead, a power-law model with a photon index of 2.4-2.5 gives a reasonable fit to the spectrum, suggesting a non-thermal origin. Together with the similarity to SN 1006, we propose that RX J1713.7-3946 is the second example, after SN 1006, of synchrotron X-ray radiation from a shell of SNRs. Since the synchrotron X-rays suggest the existence of extremely high energy charged particles in the SNR shell, our discovery should have a strong impact on the origin of cosmic X-rays.
引用
收藏
页码:L7 / L11
页数:5
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