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Using cm Observations to Constrain the Abundance of Very Small Dust Grains in Galactic Cold Cores
C. T. Tibbs, R. Paladini, K. Cleary +9
In this analysis we illustrate how the relatively new emission mechanism known as spinning dust can be used to characterize dust grains in the interstellar medium. We demonstrate t…
CARMA Observations of Galactic Cold Cores: Searching for Spinning Dust Emission
C. T. Tibbs, R. Paladini, K. Cleary +9
We present the first search for spinning dust emission from a sample of 34 Galactic cold cores, performed using the CARMA interferometer. For each of our cores we use photometric d…
Dust models post-Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium
Lapo Fanciullo, Vincent Guillet, Gonzalo Aniano +5
We compare the performance of several dust models in reproducing the dust spectral energy distribution (SED) per unit extinction in the diffuse interstellar medium (ISM). We use ou…
Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index
Melanie Köhler, Nathalie Ysard, Anthony P. Jones
Variations in the observed dust emission and extinction indicate a systematic evolution of grain properties in the transition from the diffuse interstellar medium (ISM) to denser m…
Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations
N. Ysard, M. Koehler, A. Jones +3
The Planck-HFI all-sky survey from 353 to 857GHz combined with the 100 microns IRAS show that the dust properties vary in the diffuse ISM at high Galactic latitude (1e19<NH<2.5e20…
Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
Planck Collaboration, P. A. R. Ade, N. Aghanim +195
Within ten nearby (d < 450 pc) Gould Belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane of sky, inferred fro…