17 citations · 17 across the 3 of their papers we have counts for
3 papers
astro-ph.EP2024
Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures
Wenrui Xu, Songhu Wang
In protoplanetary disks, sufficiently massive planets excite pressure bumps, which can then be preferred locations for forming new planet cores. We discuss how this loop may affect…
astro-ph.SR2023
Gravitational instability, spiral substructure, and modest grain growth in a typical protostellar disk: Modeling multi-wavelength dust continuum observation of TMC1A
Wenrui Xu, Satoshi Ohashi, Yusuke Aso +1
Embedded, Class 0/I protostellar disks represent the initial condition for planet formation. This calls for better understandings of their bulk properties and the dust grains withi…
astro-ph.EP2023★ 17 cited
Revisiting collisional dust growth in Class 0/I protostellar disks: Sweep-up can convert a few of dust into kg pebbles in 0.1 Myr
Wenrui Xu, Philip J. Armitage
Recent observations suggest that the first stages of planet formation likely take place in the Class 0/I phase of Young Stellar Object evolution, when the star and the disk are sti…