CORDIS Project
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The ORBIT-D project investigates the presence of undetected binary stars in transition discs around young stellar objects. By identifying these circumbinary discs, it aims to enhance understanding of star and planet formation processes.
Star formation begins when the densest regions in molecular clouds collapse under their own weight forming so called “young stellar objects” (YSOs), i.e. protostars surrounded by a gas+dust disc (known as “protostellar” or “protoplanetary” disc), expected to be the birth place of planets in this newly formed proto-exo-solar systems.
The advancements during the past decade in our observational capabilities revealed that 10% of the observed protostellar discs in YSOs present large (~10 –100 au) d…
UNIVERSITA DEGLI STUDI DI MILANO
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