167 citations · 1.1k across the 25 of their papers we have counts for
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On the importance of scattering at 8 microns: Brighter than you think
Charlène Lefèvre, Laurent Pagani, Michiel Min +2
Context. Extinction and emission of dust models need for observational constraints to be validated. The coreshine phenomenon has already shown the importance of scattering in the 3…
Galactic cold cores VI. Dust opacity spectral index
M. Juvela, K. Demyk, Y. Doi +13
The Galactic Cold Cores project has made Herschel observations of 116 fields where the Planck survey has found signs of cold dust emission. The fields contain sources in different…
Grain size limits derived from 3.6 μm and 4.5 μm coreshine
J. Steinacker, M. Andersen, W. -F. Thi +8
Recently discovered scattered light from molecular cloud cores in the wavelength range 3-5 μm (called "coreshine") seems to indicate the presence of grains with sizes above 0.5 μm.…
Lambda = 3 mm line survey of nearby active galaxies
Rebeca Aladro, Sergio Martín, Denise Riquelme +8
We used the IRAM 30m telescope to observe the frequency range [86-116]GHz towards the central regions of the starburst galaxies M83, M82, and NGC253, the AGNs M51, NGC1068, and NGC…
Galactic cold cores V. Dust opacity
M. Juvela, I. Ristorcelli, D. J. Marshall +14
The project Galactic Cold Cores has made Herschel observations of interstellar clouds where the Planck satellite survey has located cold and compact clumps. The sources range from…
Can we trace very cold dust from its emission alone ?
Laurent Pagani, Charlène Lefèvre, Mika Juvela +2
Context. Dust is a good tracer of cold dark clouds but its column density is difficult to quantify. Aims. We want to check whether the far-infrared and submillimeter high-resolutio…