An MSX Infrared Analysis of the Superbubble around the Giant HII Region NGC3603

Jia Wang; Yang Chen (Nanjing University)

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An MSX Infrared Analysis of the Superbubble around the Giant HII Region NGC3603

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arxiv 0907.0575 v5 pith:EJBSX5VK submitted 2009-07-03 astro-ph.GA

Jia Wang , Yang Chen (Nanjing University) This is my paper · ORCID

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keywords dominateddustemissiongiantinfraredngc3603regionsuperbubble

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Using the MSX mid-infrared observation, we reveal a 100 pc-scale superbubble surrounding the giant HII region NGC3603. We suggest that the diffuse surrounding infrared emission in bands A, C, and D is dominated by that of PAH and the emission in band E is dominated by that of dust grains. The fitted dust temperature is consistent with the heating by the central cluster's UV photons. The derived gas-to-dust mass ratio for the bubble shell is of order 10^2.

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