The Herschel 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; D. Arzoumanian; J.-Ph. Bernard; L. Deharveng; P. Didelon; J. Di Francesco; D. Elia; M. Hennemann; T. Hill; V. Könyves; J. Z. Li; P. G. Martin; Q. Nguyen Luong; N. Peretto; S. Pezzuto; D. Polychroni; H. Roussel; K. L. J. Rygl; L. Spinoglio; L. Testi; J. Tigé; R. Vavrek; D. Ward-Thompson; G. White

doi:10.1051/0004-6361/201219971

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Volume 554 (June 2013)

A&A, 554 (2013) A42

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Issue		A&A Volume 554, June 2013


Article Number		A42
Number of page(s)		12
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201219971
Published online		03 June 2013

Online material

Appendix A: Interplay between the ionized gas (Hα) and the dust

In this section, we show images combining Herschel and Hα images. The Hα image is from the UKST Hα survey (Parker et al. 2005).

	Fig. A.1 Hα image of NGC 6334 (22 × 13). The isocontours represent the Herschel-500 μm intensity (the five contours levels are from 6 Jy/beam to 656 Jy/beam in equal logarithmic steps).
Open with DEXTER

	Fig. A.2 Three-colour image (18 × 10) of NGC 6334 with 500 μm data in red, 160 μm data in green, and 70 μm data in blue. The Hα isocontours are overlaid (the five contours levels are, in arbitrary units, from 6000 to 15 000 on a linear scale).
Open with DEXTER

© ESO, 2013

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