Spectral energy distributions of H ii regions in M 33 (HerM33es)

M. Relaño; S. Verley; I. Pérez; C. Kramer; D. Calzetti; E. M. Xilouris; M. Boquien; J. Abreu-Vicente; F. Combes; F. Israel; F. S. Tabatabaei; J. Braine; C. Buchbender; M. González; P. Gratier; S. Lord; B. Mookerjea; G. Quintana-Lacaci; P. van der Werf

doi:10.1051/0004-6361/201220073

Free Access

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.

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	Fig. A.2 Same as Fig. A.1 for H ii region number 48 classified as clear shell.
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	Fig. A.3 Same as Fig. A.1 for H ii region number 23 classified as filled.
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	Fig. A.4 Same as Fig. A.1 for H ii region number 35 classified as filled.
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Appendix B: Tables

Table B.1

Selection of Hii regions.

Table B.2

Fluxes of our set of H ii regions in mJy within the apertures shown in Table B.1.

Table B.3

Dust properties of H ii regions.

© ESO, 2013

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