The Citing articles tool gives a list of articles citing the current article. The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
C/O ratios in self-gravitating protoplanetary discs with dust evolution
Tamara Molyarova, Eduard Vorobyov and Vitaly Akimkin Publications of the Astronomical Society of Australia 42 (2025) https://doi.org/10.1017/pasa.2024.126
Constraints on PDS 70 b and c from the dust continuum emission of the circumplanetary discs considering in situ dust evolution
Surviving the heat: multiwavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles
Adrien Houge, Enrique Macías and Sebastiaan Krijt Monthly Notices of the Royal Astronomical Society 527(4) 9668 (2023) https://doi.org/10.1093/mnras/stad3758
An inflationary disk phase to explain extended protoplanetary dust disks
Modelling the evolution of silicate/volatile accretion discs around white dwarfs
Ayaka Okuya, Shigeru Ida, Ryuki Hyodo and Satoshi Okuzumi Monthly Notices of the Royal Astronomical Society 519(2) 1657 (2022) https://doi.org/10.1093/mnras/stac3522
A “no-drift” runaway pile-up of pebbles in protoplanetary disks
A global two-layer radiative transfer model for axisymmetric, shadowed protoplanetary disks
Satoshi Okuzumi, Takahiro Ueda and Neal J Turner Publications of the Astronomical Society of Japan 74(4) 828 (2022) https://doi.org/10.1093/pasj/psac040
Effective dust growth in laminar circumplanetary discs with magnetic wind-driven accretion
Dust accumulation near the magnetospheric truncation of protoplanetary discs around T Tauri stars
Rixin Li(李日新), Yi-Xian Chen(陈逸贤) and Douglas N C Lin(林潮) Monthly Notices of the Royal Astronomical Society 510(4) 5246 (2022) https://doi.org/10.1093/mnras/stab3677
A “no-drift” runaway pile-up of pebbles in protoplanetary disks in which midplane turbulence increases with radius