CORDIS Project
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This research project investigates the formation of high-mass stars by examining the physical conditions in their surrounding gas and dust. It utilizes advanced infrared observations to understand the mechanisms influencing star formation.
The classic problem in the formation of high-mass stars is that, for all stars above ~20 Msun, the outward force exerted by the stars radiation on the dusty circumstellar gas should be capable of reversing or halting accretion flows.
Core fragmentation, pressure from the expanding ionised gas, magnetic fields and mass loss through stellar winds, all work against the effects of gravity, thereby restricting the final stellar mass.
Advances in theoretical models, aided by numerical simulations (e.g…
THE UNIVERSITY OF HERTFORDSHIRE HIGHER EDUCATION CORPORATION
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