Iron and nickel line diagnostics for the galactic center diffuse emission

Publications of the Astronomical Society of Japan

Volumn 59, Issue 1 SPEC. ISS., 2007, Pages

  Koyama, Katsuji ^a   Hyodo, Yoshiaki ^a   Inui, Tatsuya ^a   Nakajima, Hiroshi ^a   Matsumoto, Hironori ^a   Tsuru, Takeshi Go ^a   Takahashi, Tadayuki ^b   Maeda, Yoshitomo ^b   Yamazaki, Noriko Y ^b   Murakami, Hiroshi ^b   Yamauchi, Shigeo ^c   Tsuboi, Yohko ^d   Senda, Atsushi ^e   Kataoka, Jun ^f   Takahashi, Hiromitsu ^g   Holt, Stephen S ^h   Brown, Gregory V ⁱ  

^a KYOTO UNIVERSITY   (Japan)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c IWATE UNIVERSITY   (Japan)

^d CHUO UNIVERSITY   (Japan)

^e INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

^f Tokyo Institute of Technology ^*  (Japan)

^g HIROSHIMA UNIVERSITY   (Japan)

^h FRANKLIN W OLIN COLLEGE OF ENGINEERING   (United States)

ⁱ LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

Author keywords

Galaxy: center; ISM: abundances; ISM: dust, extinction; X ray spectra

Indexed keywords

COLLISIONAL PLASMAS; ELECTROMAGNETIC WAVE EMISSION; IONIZATION OF GASES; IRON; IRON COMPOUNDS; NICKEL COMPOUNDS; X RAY ANALYSIS; GALAXIES;

DIFFUSE EMISSION; DUST EXTINCTIONS; GALACTIC CENTER; GALAXY CENTER; ISM: ABUNDANCE; ISM: DUST, EXTINCTION; ISM:DUST; KΑ; X RAY SPECTRUM; X-RAY IMAGING SPECTROMETERS;

NICKEL;

EID: 34047167899     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/59.sp1.s245     Document Type: Article

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