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Title:
mid- to far-infrared mapping spectroscopy of galactic star-forming regions with ISO, spitzer, and AKARI
Authors:
Okada, Y.; Onaka, T.; Miyata, T.; Okamoto, Y. K.; Sakon, I.; Shibai, H.; Takahashi, H.; Kawada, M.; Murakami, N.; Nakagawa, T.; Ootsubo, T.; Yasuda, A.
Affiliation:
AA(Institute of Space and Astronautical Science, JAXA, Japon;; ), AB(University of Tokyo), AC(University of Tokyo), AD(Ibaraki University), AE(University of Tokyo), AF(Nagoya University), AG(Gunma Astronomical Observatory), AH(Nagoya University), AI(Bisei Astronomical Observatory), AJ(Institute of Space and Astronautical Science, JAXA, Japon;), AK(Nagoya University), AL(Institute of Space and Astronautical Science, JAXA, Japon;)
Publication:
EAS Publications Series, Volume 31, 2008, pp.191-192
Publication Date:
00/2008
Origin:
EDP Sciences
DOI:
10.1051/eas:0831041
Bibliographic Code:
2008EAS....31..191O

Abstract

We report the results of mid- to far-infrared spectroscopic observations of Galactic star-forming regions with ISO, Spitzer, and AKARI. Owing to the high sensitivity of the IRS onboard Spitzer, we detected [Si II] 35 μm, [Fe II] 26 μm, and [Fe III] 23 μm lines widely in low-density star-forming regions, and derived gas-phase Si and Fe abundances as 3 100% and <22%, respectively. With the FTS onboard AKARI, we obtained the spatial distribution of the [O III] 88 μm emission in two star-forming regions.
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