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Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel
Jeremy Chastenet, Caroline Bot, Karl D. Gordon +4
Dust modeling is crucial to infer dust properties and budget for galaxy studies. However, there are systematic disparities between dust grain models that result in corresponding sy…
DustPedia - A Definitive Study of Cosmic Dust in the Local Universe
J. I. Davies, M. Baes, S. Bianchi +20
The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…
The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus
S. Bianchi, C. Giovanardi, M. W. L. Smith +22
We study the correlation between far-infared/submm dust emission and atomic gas column density in order to derive the properties of the high Galactic latitude, low density, Milky W…
Stellar classification of CoRoT targets
C. Damiani, J. -C. Meunier, C. Moutou +4
The CoRoT faint stars channel observed about 163 600 targets to detect transiting planetary companions. Because CoRoT targets are faint (11< r <16) and close to the galactic plane,…
Mantle formation, coagulation and the origin of cloud/core-shine: II. Comparison with observations
N. Ysard, M. Koehler, A. P. Jones +3
Many dense interstellar clouds are observable in emission in the near-IR, commonly referred to as "Cloudshine", and in the mid-IR, the so-called "Coreshine". These C-shine observat…
Mantle formation, coagulation and the origin of cloud/core shine: I. Modelling dust scattering and absorption in the infra-red
A. P. Jones, M. Koehler, N. Ysard +3
Context. The observed cloudshine and coreshine (C-shine) have been explained in terms of grain growth leading to enhanced scatter- ing from clouds in the J, H and K photometric ban…