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Discovery of Non Thermal X-Rays from the Northwest Shell of the New SNR RX J1713.7-3946: The Second SN1006 ?

Katsuji Koyama Kenzo Kinugasa Keiichi Matsuzaki Mamiko Nis Physics, K. University, Department of Earth, Space Science, Osaka University, D. Physics, U. O. T. I. O. Space, Astronautical Science et al.

1997

59 citations

Abstract

We report 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 reasonable fit to the spectrum, suggesting a non-thermal origin. Together with the similarity to SN1006, we propose that RX J1713.7 − 3946 is the second example, after SN1006, of a synchrotron X-ray radiation from a shell of SNRs. Since the synchrotron X-rays suggest existence of extremely high energy charged particles in the SNR shell, our discovery should have strong impact on the origin of the cosmic X-rays.

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