| Issue |
A&A
Volume 552, April 2013
|
|
|---|---|---|
| Article Number | A140 | |
| Number of page(s) | 25 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201220073 | |
| Published online | 17 April 2013 | |
Online material
Appendix A: Two-dimensions multi-wavelength projected profiles of H ii regions
 |
Fig. A.1
Emission line profiles for H ii region 87 classified as clear shell in the horizontal (left) and vertical (right) directions. For clarity, the profiles are separated into three panels (top: Hα, FUV, NUV; middle: 3.6 μm, 4.5 μm, 5.8 μm, 8.0 μm; bottom: 24 μm, 70 μm, 100 μm, 160 μm, 250 μm). The small box in top left corner in each panel shows the location of the profile overlaid on the region, the images correspond to Hα, 4.5 μm, and 250 μm for the top, middle, and bottom panels, respectively. All the profiles are normalised to their maxima. The Hα profile is depicted in grey in all the panels for reference. |
| Open with DEXTER | |
 |
Fig. A.2
Same as Fig. A.1 for H ii region number 48 classified as clear shell. |
| Open with DEXTER | |
 |
Fig. A.3
Same as Fig. A.1 for H ii region number 23 classified as filled. |
| Open with DEXTER | |
 |
Fig. A.4
Same as Fig. A.1 for H ii region number 35 classified as filled. |
| Open with DEXTER | |
Appendix B: Tables
Selection of Hii regions.
Dust properties of H ii regions.
© ESO, 2013
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