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- W1991228082 abstract "Abstract We explore the physical characteristics of young stellar clusters in the Antennae by combining recent ground- and space-based mid-infrared observations with a newly developed set of diagnostic diagrams. Spitzer data give an overview of the star-forming regions extending over hundreds of parsecs, showing a dominant diffuse ISM component with a density of 10 2 cm −3 plus a small fraction of very compact material (10 6 cm −3 ). With its higher spatial resolution VISIR gives a close-up view of the latter component. Its emission line ratios suggest that these regions are fundamentally different from local star-forming regions. Instead of having small isolated UCHII regions, as in local star-forming regions, the average density of the medium of the whole region falls in the (ultra)compact regime, exceeding 10 4 cm −3 over tens of parsecs." @default.
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- W1991228082 date "2006-08-01" @default.
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- W1991228082 title "UCHII regions in the Antennae" @default.
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- W1991228082 doi "https://doi.org/10.1017/s1743921307002645" @default.
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