Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud

F. Galliano; S. Hony; J.-P. Bernard; C. Bot; S. C. Madden; J. Roman-Duval; M. Galametz; A. Li; M. Meixner; C. W. Engelbracht; V. Lebouteiller; K. Misselt; E. Montiel; P. Panuzzo; W. T. Reach; R. Skibba

doi:10.1051/0004-6361/201117952

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Volume 536 (December 2011)

A&A, 536 (2011) A88

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Fig. A.1

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Comparison of the grain properties of our two models. The top panels show the opacity of the two mixtures. The grey dash lines show long wavelength fits of these opacities, with empirical laws ∝ ν^β. The bottom panel compares the SEDs of the two grain mixtures illuminated by the ISRF of the diffuse Galactic ISM (U = 1).

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