27–30 Apr 2015
Europe/Berlin timezone

Laboratory measurements of the far-infrared to millimeter wave dust opacity.

29 Apr 2015, 11:45
10m
Contributed talk Session2, Wednesday

Speaker

Pierre Mohr (Friedrich Schiller University Jena)

Description

P. Mohr, F. Lewen, H. Mutschke In this project, we have synthesized glassy Mg-Fe silicates as interstellar-dust analog materials and have determined their absorption/emission coefficients at low temperatures in the wavelength range from 50 micrometers to 4 millimeters. We have found a strong dependence of the dust opacity on the temperature and a moderate depencence on the chemical composition, i.e. the content of divalent and trivalent iron. A dependence on the grain size is also detected, which could point to an influence of additional defects created by milling. In the new project phase, we will continue with similar measurements on carbonaceous materials.

Author

Pierre Mohr (Friedrich Schiller University Jena)

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