CORDIS Project
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This project investigates the formation of high-mass stars by studying gas filaments in the Milky Way. Using advanced observational techniques, it aims to understand the processes that lead to the creation of these massive stars and how they differ from low-mass star formation.
High-mass stars drive the physical and chemical evolution of the Universe.
However, the origin of these massive objects is largely controversial.
Three key questions remain under debate: a) Which physical processes determine the formation of high-mass stars? b) How do these stars get their large masses? c) Do high-mass stars form in a similar way to their low-mass counterparts?
Galactic surveys link the origin of high-mass stars to the initial properties of their gas embryos.
Using the Atacama L…
UNIVERSITAT WIEN
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Germany, MUNCHEN
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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