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A Suzaku Observation of the Low-Ionization Fe-Line Emission from RCW 86
Masaru Ueno, Rie Sato, Jun Kataoka +14
The newly operational X-ray satellite Suzaku observed the southwestern quadrant of the supernova remnant (SNR) RCW 86 in February 2006 to study the nature of the 6.4 keV emission l…
Monte-Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis
Y. Ishisaki, Y. Maeda, R. Fujimoto +31
We have developed a framework for the Monte-Carlo simulation of the X-Ray Telescopes (XRT) and the X-ray Imaging Spectrometers (XIS) onboard Suzaku, mainly for the scientific analy…
Suzaku Observations of HESS J1616-508: Evidence for a Dark Particle Accelerator
Hironori Matsumoto, Masaru Ueno, Aya Bamba +15
We observed the bright unidentified TeV gamma-ray source HESS J1616-508 with the X-ray Imaging Spectrometers onboard the Suzaku satellite. No X-ray counterpart was found to a limit…
Discovery of a Compact X-ray Source in the LMC Supernova Remnant N23 with Chandra
Asami Hayato, Aya Bamba, Toru Tamagawa +1
An X-ray compact source was discovered with Chandra in a supernova remnant (SNR) N23, located in the Large Magellanic Cloud. The compact source (CXOU J050552.3-680141) is seen in o…
The X-ray synchrotron emission of RCW 86 and the implications for its age
Jacco Vink, Johan Bleeker, Kurt van der Heyden +3
We report here X-ray imaging spectroscopy observations of the northeastern shell of the supernova remnant RCW 86 with Chandra and XMM-Newton. Along this part of the shell the domin…
A Detailed Observation of a LMC Supernova Remnant DEM L241 with XMM-Newton
Aya Bamba, Masaru Ueno, Hiroshi Nakajima +2
We report on an {\it XMM-Newton} observation of the supernova remnant (SNR) \object{DEM L241} in the Large Magellanic Cloud. In the soft band image, the emission shows an elongated…
TeV Gamma-Rays from Old Supernova Remnants
Ryo Yamazaki, Kazunori Kohri, Aya Bamba +3
We study the emission from an old supernova remnant (SNR) with an age of around 10^5 yrs and that from a giant molecular cloud (GMC) encountered by the SNR. When the SNR age is aro…