Multi-generation massive star-formation in NGC 3576

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Multi-generation massive star-formation in NGC 3576

Context: Recent 1.2-mm continuum observations have shown the giant H II region NGC 3576 to be embedded in the centre of an extended filamentary dust-cloud. The bulk of the filament away from the H II region contains a number of clumps seen only at (sub-)millimetre wavelengths. Infrared and radio obs...

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Bibliographic Details
Main Authors:	Purcell, C., Minier, V., Longmore, S., André, P., Walsh, Andrew, Jones, P., Herpin, F., Hill, T., Cunningham, M., Burton, M.
Format:	Journal Article
Published:	EDP Sciences 2009
Subjects:	ISM: molecules stars: pre-mainsequence HII regions radio ISM: abundances lines: ISM stars: formation
Online Access:	http://www.aanda.org/articles/aa/pdf/2009/34/aa11358-08.pdf http://hdl.handle.net/20.500.11937/36731

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