@article{
 title = {Observation of Fe-line emission from Sagittarius B2 - Evidence for past activities of our galaxy},
 type = {article},
 year = {2000},
 identifiers = {[object Object]},
 pages = {579-582},
 volume = {25},
 websites = {http://linkinghub.elsevier.com/retrieve/pii/S0273117799008042},
 month = {1},
 publisher = {Pergamon},
 day = {1},
 id = {e32cf0f7-0547-3280-adcf-288e3c80960a},
 created = {2019-11-05T08:27:59.922Z},
 accessed = {2018-01-30},
 file_attached = {true},
 profile_id = {ec4888e4-cd9f-3ee0-90a1-39a024d1537d},
 last_modified = {2022-07-15T21:49:02.496Z},
 read = {true},
 starred = {false},
 authored = {true},
 confirmed = {true},
 hidden = {false},
 citation_key = {murakami00b},
 source_type = {article},
 folder_uuids = {9989056f-58f0-4daf-a99f-4779f0cdd416,5a859072-32ae-4559-8859-863b99a8e32c},
 private_publication = {false},
 abstract = {We present the ASCA results of imaging spectroscopy of the giant molecular cloud Sgr B2. The X-ray spectrum is found to be very peculiar; it exhibits a strong emission line at 6.4 keV, a low energy cutoff below 4 keV and a pronounced edge-structure at 7.1 keV. The X-ray image is extended and its peak position is shifted in the direction of the Galactic center by about 1-2 arcminute from the core of the molecular cloud. The X-ray spectrum and morphology are well reproduced by a scenario that X-rays from a source located at the Galactic center side are scattered by the molecular cloud Sgr B2, and come into our line of sight. Thus Sgr B2 may be called an X-ray reflection nebula. © 2000 COSPAR. Published by Elsevier Science Ltd.},
 bibtype = {article},
 author = {Murakami, H. and Koyama, K. and Maeda, Y. and Sakano, M. and Nishiuchi, M. and Tsujimoto, M.},
 journal = {Advances in Space Research},
 number = {3-4}
}

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