CORDIS Project
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This project aims to create a detailed map of the Perseus Spiral Arm of the Milky Way, focusing on giant molecular clouds that are crucial for star formation. By analyzing data from various gas components, the project will compare cloud properties across different environments to enhance understanding of star formation…
Giant molecular clouds (GMCs) are the principal sites of star formation.
The derivation of cloud properties are complicated by their large spread in distance along the line of sight.
Consequently, to gain insight into the GMCs' physical states one compares parsec-sized clouds of a few hundred solar masses in the solar neighbourhood to the largest, million-solar-mass GMCs in the distant Milky Way.
The main goal of my project is to produce the first map of the Perseus Spiral Arm in our outer Galax…
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