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- W2152962859 abstract "We surveyed spatial profiles of the Fe K |$alpha $| lines in the Galactic center diffuse X-rays (GCDX), including the transient region from the GCDX to the Galactic ridge X-ray emission (GRXE), with the Suzaku satellite. We resolved Fe K |$alpha $| line complex into three lines of Fe I, Fe XXV, and Fe XXVI K |$alpha $| , and obtained their spatial intensity profiles with a resolution of |$sim $| 0 |$^circ!!!.$| 1. We compared the Fe XXV K |$alpha $| profile with a stellar mass distribution (SMD) model made from near infrared observations. The intensity profile of Fe XXV K |$alpha $| was nicely fitted with the SMD model in the GRXE region, while that in the GCDX region showed a 3.8 |$ pm $| 0.3 (0 |$^circ!!!.$| 2 |$<$||$vert lvert$||$<$| 1 |$^circ!!!.$| 5) or 19 |$ pm $| 6 ( |$vert lvert$||$<$| 0 |$^circ!!!.$| 2) times excess over the best-fit SMD model in the GRXE region. Thus, Fe XXV K |$alpha $| in the GCDX is hardly explained by the same origin of the GRXE. In the case of a point-source origin, a new population with the extremely strong Fe XXV K |$alpha $| line is required. An alternative possibility is that the majority of the GCDX is truly diffuse optically thin thermal plasma." @default.
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- W2152962859 date "2011-11-25" @default.
- W2152962859 modified "2023-09-23" @default.
- W2152962859 title "Global Distribution of Fe Kα Lines in the Galactic Center Region Observed with the Suzaku Satellite" @default.
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- W2152962859 doi "https://doi.org/10.1093/pasj/63.sp3.s903" @default.
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