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1-20. The Properties of dust emission in the Galactic center region revealed by FIS-FTS observations. SW:blue LW:black. ○ A. Yasuda, H. Kaneda, A. Takahashi (Nagoya University), M. Kawada, T. Nakagawa (ISAS/JAXA), Y. Okada (Köln University), - PowerPoint PPT Presentation
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Cold dust
○A. Yasuda, H. Kaneda, A. Takahashi (Nagoya University), M. Kawada, T. Nakagawa (ISAS/JAXA), Y. Okada (Köln University),
H. Takahashi (NAOJ), N. Murakami (Bisei Observatory)
SW:blueLW:black
A two temperature greybody model reproduces the spectrum very well.
1-20
Warm dust
Contours: [OIII] line emission
Contours: Total CO(J=1-0)
The warm dust and the [OIII] line emission (88um) are well correlated with each other, which are associated with the Arches and the Quintuplet cluster.However, the cold dust is not associated with either the Arches or the Quintuplet cluster.
1-20
Dust mass [M_solar]Warm dust
Cold dust
Arches 26 2.1×103
Quintuplet
15 1.3×103
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