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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Table A.1

Submillimeter properties of our dust compositions.

	“Standard model”	“AC model”

β	2	1.7
κ_abs(160 μm)	1.4m² kg^-1	1.6m² kg^-1

Notes. The two parameters β and κ_abs(160 μm) are the parameters to approximate our dust opacities (Fig. A.1) with Eq. (A.1).

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