Speaker
Dr
Maud Galametz
(CEA Saclay)
Description
In this review, I will give an overview of the properties of dust (spatial distribution, composition, heating sources) in the ISM of nearby galaxies and in the Milky Way. I will discuss the main spectral energy distributions fitting techniques to model the ISM dust and their caveats. I will also discuss the need for dust models including an evolution of dust grains in the ISM to explain the current observables in emission or extinction.
Primary author
Dr
Maud Galametz
(CEA Saclay)
