{"paper":{"title":"Discoveries of Diffuse Iron Line Sources from the Sgr B Region","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Chan Yang Soong, Hironori Matsumoto, Hiroshi Murakami, Kai-Wing, Katsuji Koyama, Shigeo Yamauchi, Steven E. Kissel, Takeshi Go Tsuru, Tatsuya Inui, Yoshiaki Hyodo, Yoshitomo Maeda","submitted_at":"2006-09-12T05:33:00Z","abstract_excerpt":"The radio complex Sgr B region is observed with the X-Ray Imaging Spectrometers (XIS) on board Suzaku. This region exhibits diffuse iron lines at 6.4, 6.7 and 6.9 keV, which are K$\\alpha$ lines of Fe \\emissiontype{I} (neutral iron), Fe\\emissiontype{XXV} (He-like iron) and Fe\\emissiontype{XXVI} (H-like iron), respectively. The high energy resolving power of the XIS provides the separate maps of the K-shell transition lines from Fe\\emissiontype{I} (6.4 keV) and Fe\\emissiontype{XXV} (6.7 keV). Although the 6.7 keV line is smoothly distributed over the Sgr B region, a local excess is found near at"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609310","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}