Exploring the possibility of Peter Pan discs across stellar mass
Monthly Notices of the Royal Astronomical Society(2021)
Abstract
Recently, several accreting M dwarf stars have been discovered with ages far exceeding the typical protoplanetary disc lifetime. These ‘Peter Pan discs’ can be explained as primordial discs that evolve in a low-radiation environment. The persistently low masses of the host stars raise the question whether primordial discs can survive up to these ages around stars of higher mass. In this work we ex...
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Key words
accretion, accretion discs,protoplanetary discs
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