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Mid- to far-infrared mapping spectroscopy of galactic star-forming regions with ISO, spitzer, and AKARI

Published online by Cambridge University Press:  04 October 2008

Y. Okada
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japon
T. Onaka
Affiliation:
University of Tokyo
T. Miyata
Affiliation:
University of Tokyo
Y.K. Okamoto
Affiliation:
Ibaraki University
I. Sakon
Affiliation:
University of Tokyo
H. Shibai
Affiliation:
Nagoya University
H. Takahashi
Affiliation:
Gunma Astronomical Observatory
M. Kawada
Affiliation:
Nagoya University
N. Murakami
Affiliation:
Bisei Astronomical Observatory
T. Nakagawa
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japon
T. Ootsubo
Affiliation:
Nagoya University
A. Yasuda
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japon
Corresponding
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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.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

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References

Kawada, M., et al., 2007, PASJ, 59, 389 CrossRef
Okada, Y., et al., submitted
Okada, Y., Onaka, T., Nakagawa, T., Shibai, H., Tomono, D., & Yui, Y.Y., 2006, ApJ, 640, 383 CrossRef
Okada, Y., Onaka, T., Shibai, H., & Doi, Y., 2003, A&A, 412, 199

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Mid- to far-infrared mapping spectroscopy of galactic star-forming regions with ISO, spitzer, and AKARI
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