Multi-generation massive star-formation in NGC 3576

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

Internet

http://www.aanda.org/articles/aa/pdf/2009/34/aa11358-08.pdf
http://hdl.handle.net/20.500.11937/36731

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