CORDIS Project
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This project investigates how external heating from massive stars affects the formation of planets in protoplanetary discs. By modeling mass-loss rates and comparing them to observations, it aims to enhance our understanding of planet formation in environments typical of star formation.
Star and planet formation typically occurs in star forming regions more massive than the nearby, low-mass regions that have been the main focus of observational studies of protoplanetary discs.
In massive regions, irradiation by neighbouring massive stars can heat this protoplanetary disc of dust and gas, from which planets form.
This heating drives thermal winds that extract dust and gas, reducing the mass available for planet formation.
In typical star and planet forming environments, these wi…
OBSERVATOIRE DE LA COTE D'AZUR (OCA)
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France, Nice
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
United Kingdom, London
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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