The<i>Herschel</i>view of the massive star-forming region NGC 6334

D. Russeil, N. Schneider, L. D. Anderson, A. Zavagno, S. Molinari, P. Persi, S. Bontemps, F. Motte, V. Ossenkopf, Ph. André,

Astronomy and Astrophysics · 2013 · 96 citations · 80 references

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Abstract

Aims. Fundamental to any theory of high-mass star formation are gravity and turbulence. Their relative importance, which probably changes during cloud evolution, is not known. By investigating the spatial and density structure of the high-mass star-forming complex NGC 6334 we aim to disentangle the contributions of turbulence and gravity.

References

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