CORDIS Project
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This project studies the role of interstellar dust in star-forming regions, focusing on its physical properties and impact on star formation rates. It utilizes multiwavelength observations to understand dust's contribution to the dynamics of interstellar gas.
Understanding the formation and evolution of a galaxy requires the knowledge of the properties of its stellar population and its star formation activity.
The presence of dust in the interstellar medium is fundamental in the star formation process, and is a by-product of that process, which makes the dust itself a tracer of the star formation rate within galaxies.
The interstellar dust absorbs the ultraviolet (UV) radiation coming from the stars and re-emits it in the infrared (IR).
The correcti…
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