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The Nature of Unresolved Soft X-ray Emission from the Galactic Disk
K. Masui, K. Mitsuda, N. Y. Yamasaki +4
Although about 40% of the soft X-ray background emission in 0.4 to 1 keV range has extragalactic origins and thus is totally blocked by the Galactic absorption in midplane directio…
Iron Emission Lines on the Galactic Ridge Observed with Suzaku
Shigeo Yamauchi, Ken Ebisawa, Yasuo Tanaka +5
In order to elucidate origin of the Galactic Ridge X-ray Emission, we analyzed Suzaku data taken at various regions along the Galactic plane and studied their Fe-K emission line fe…
The NeXT Mission
T. Takahashi, R. Kelley, K. Mitsuda +28
The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2…
On the lack of strong O-line excess in the Coma cluster outskirts from Suzaku
Yoh Takei, Eric D. Miller, Joel N. Bregman +6
About half of the baryons in the local Universe are thought to reside in the so-called warm-hot intergalactic medium (WHIM) at temperatures of 0.1-10 million K. Thermal soft excess…