Dispersal of protoplanetary disks by the combination of magnetically driven and photoevaporative winds

12 Jan 2020 Kunitomo Masanobu Suzuki Takeru K. Inutsuka Shu-ichiro

We investigate the roles of magnetically driven disk wind (MDW) and thermally driven photoevaporative wind (PEW) in the long-time evolution of protoplanetary disks. We start simulations from the early phase in which the disk mass is $0.118\,{\mathrm{M}_{\odot}}$ around a $1\,{\mathrm{M}_{\odot}}$ star and track the evolution until the disk is completely dispersed... (read more)

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  • EARTH AND PLANETARY ASTROPHYSICS
  • SOLAR AND STELLAR ASTROPHYSICS