Measuring the Broad-Band X-Ray Spectrum from 400eV to 40keV in the Southwest Part of the Supernova Remnant RXJ1713.7 $-$ 3946

• Published in: Publications of the Astronomical Society of Japan 2008-02, Vol.60 (sp1), p.S131-S140
• Main Authors: Takahashi, Tadayuki, Tanaka, Takaaki, Uchiyama, Yasunobu, Hiraga, Junko S., Nakazawa, Kazuhiro, Watanabe, Shin, Bamba, Aya, Hughes, John P., Katagiri, Hideaki, Kataoka, Jun, Kokubun, Motohide, Koyama, Katsuji, Mori, Koji, Petre, Robert, Takahashi, Hiromitsu, Tsuboi, Yoko
• Format: Article
• Language: English
• ISSN: 0004-6264; 2053-051X
• DOI: 10.1093/pasj/60.sp1.S131

We report on results from Suzaku broadband X-ray observations of the southwest part of the galactic supernova remnant (SNR) RXJ1713.7 $-$ 3946 with an energy coverage of 0.4-40keV. The X-ray spectrum, presumably of synchrotron origin, is known to be completely lineless, making this SNR ideally suited for a detailed study of the X-ray spectral shape formed through efficient particle acceleration at high-speed shocks. With a sensitive hard X-ray measurement from the HXD PIN aboard Suzaku, we determined the hard X-ray spectrum in the 12-40keV range to be described by a power law with photon index of $\Gamma =$ 3.2 $\pm$ 0.2, significantly steeper than the soft X-ray index of $\Gamma =$ 2.4 $\pm$ 0.05 measured previously with ASCA and other missions. We find that a simple power law fails to describe the full spectral range of 0.4-40keV, and instead a power-law with an exponential cutoff with a hard index of $\Gamma =$ 1.50 $\pm$ 0.09 and a high-energy cutoff of $\epsilon_{\rm c} =$ 1.2 $\pm$ 0.3keV formally provides an excellent fit over the full bandpass. If we use the so-called SRCUT model, as an alternative model, it gives a best-fit rolloff energy of $\epsilon_{\rm roll}$ $=$ 0.95 $\pm$ 0.04keV. Together with the TeV $\gamma$ -ray spectrum, ranging from 0.3 to 100TeV, recently obtained by HESS observations, our Suzaku observations of RXJ1713.7 $-$ 3946 provide stringent constraints on the highest-energy particles accelerated in a supernova shock.