The earliest phases of high-mass star formation: the NGC 6334-NGC 6357 complex

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The earliest phases of high-mass star formation: the NGC 6334-NGC 6357 complex

Context. Our knowledge of high-mass star formation has been mainly based on follow-up studies of bright sources found by IRAS, and has thus been incomplete for its earliest phases, which are inconspicuous at infrared wavelengths. With a new generation of powerful bolometer arrays, unbiased large-sca...

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Bibliographic Details
Main Authors:	Russeil, D., Zavagno, A., Motte, F., Schneider, N., Bontemps, S., Walsh, Andrew
Format:	Journal Article
Published:	EDP Sciences 2010
Subjects:	radio lines: general H ii regions dust submillimeter: ISM extinction radio continuum: ISM stars: formation
Online Access:	http://www.aanda.org/articles/aa/abs/2010/07/aa13632-09/aa13632-09.html http://hdl.handle.net/20.500.11937/10017

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