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...
| Main Authors: | , , , , , |
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| Format: | Journal Article |
| Published: |
EDP Sciences
2010
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| Subjects: | |
| Online Access: | http://www.aanda.org/articles/aa/abs/2010/07/aa13632-09/aa13632-09.html http://hdl.handle.net/20.500.11937/10017 |