Skip to main content Accessibility help
×
Home

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

  • C. Kramer, S. Aalto, R. Simon, Y. Okada (a1), T. Onaka (a2), T. Miyata (a2), Y.K. Okamoto (a3), I. Sakon (a2), H. Shibai (a4), H. Takahashi (a5), M. Kawada (a4), N. Murakami (a6), T. Nakagawa (a1), T. Ootsubo (a4) and A. Yasuda (a1)...

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.

Copyright

Corresponding author

References

Hide All
[1] Kawada, M., et al., 2007, PASJ, 59, 389
[2] Okada, Y., et al., submitted
[3] Okada, Y., Onaka, T., Nakagawa, T., Shibai, H., Tomono, D., & Yui, Y.Y., 2006, ApJ, 640, 383
[4] Okada, Y., Onaka, T., Shibai, H., & Doi, Y., 2003, A&A, 412, 199

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

  • C. Kramer, S. Aalto, R. Simon, Y. Okada (a1), T. Onaka (a2), T. Miyata (a2), Y.K. Okamoto (a3), I. Sakon (a2), H. Shibai (a4), H. Takahashi (a5), M. Kawada (a4), N. Murakami (a6), T. Nakagawa (a1), T. Ootsubo (a4) and A. Yasuda (a1)...

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed