Spatially resolving the dust properties and submillimetre excess in M 33
Context. The relative abundance of the dust grain types in the interstellar medium is directly linked to physical quantities that trace the evolution of galaxies. Because of the poor spatial resolution of the infrared and submillimetre data, we are able to study the dependence of the resolved infrared spectral energy distribution (SED) across
Relaño, M. et al.
Fecha de publicación:
5
2018