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Suzaku Detection of Diffuse Hard X-Ray Emission outside Vela X
Satoru Katsuda, Koji Mori, Robert Petre +9
Vela X is a large, 3x2 degrees, radio-emitting pulsar wind nebula (PWN) powered by the Vela pulsar in the Vela supernova remnant. Using four Suzaku/XIS observations pointed just ou…
Possible Charge-Exchange X-Ray Emission in the Cygnus Loop Detected with Suzaku
Satoru Katsuda, Hiroshi Tsunemi, Koji Mori +8
X-ray spectroscopic measurements of the Cygnus Loop supernova remnant indicate that metal abundances throughout most of the remnant's rim are depleted to about 0.2 times the solar…
X-Ray Spectrum of a Peculiar Supernova Remnant G359.1-0.5
Takao Ohnishi, Katsuji Koyama, Takeshi Go Tsuru +3
We present the Suzaku results of a supernova remnant (SNR), G359.1-0.5 in the direction of the Galactic center region. From the SNR, we find prominent K-shell lines of highly ioniz…