Research Project
Grant-in-Aid for Scientific Research (C)
Using the Suzaku data observed in the Galactic center, Galactic plane, and Galactic bulge regions, I studied properties of Fe-K emission lines of the Galactic diffuse X-ray emission. The ratios of 6. 97keV/6. 7 keV in the Galactic center and the Galactic bulge regions are systematically larger than that of the Galactic plane. The observed Fe emission line cannot be reproduced by a spectral model for active star binaries and white dwarf binaries. We also studied newly discovered X-ray sources and supernova remnants.
All 2012 2011 2010 2009
All Journal Article (6 results) (of which Peer Reviewed: 6 results) Presentation (10 results)
Publ. Astron. Soc. Japan
Volume: 63 Pages: 957-961
10030719265
Publications of Astronomical Society of Japan
Volume: 63
Volume: 62 Pages: 1249-1259
10027724045
Publ. Astron. Soc.
Volume: 62 Pages: 219-224
10026714405