Why do protoplanetary disks appear not massive enough to form the known exoplanet population?
A&A, 618 (2018) L3
Published online: 2018-10-11
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Revisiting Collisional Dust Growth in Class 0/I Protostellar Disks: Sweep-up Can Convert a Few 10 M ⊕ of Dust into Kilogram Pebbles in 0.1 Myr
Wenrui Xu and Philip J. ArmitageThe Astrophysical Journal 946 (2) 94 (2023)
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Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. II. Dust-ring Formation Mediated by Backreaction and Fragmentation
Ryosuke T. Tominaga, Hidekazu Tanaka, Hiroshi Kobayashi and Shu-ichiro InutsukaThe Astrophysical Journal 940 (2) 152 (2022)
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TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID
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The accretion of planet Earth
Alex N. Halliday and Robin M. CanupNature Reviews Earth & Environment 4 (1) 19 (2022)
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Demographics of Exoplanetary Systems
Sean N. Raymond and Alessandro MorbidelliAstrophysics and Space Science Library, Demographics of Exoplanetary Systems 466 3 (2022)
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Dust Resurgence in Protoplanetary Disks Due to Planetesimal–Planet Interactions
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The terrestrial planet formation around M dwarfs: insitu, inward migration, or reversed migration
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The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. VI. Insights from Radiative Transfer Modeling
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The mass and size of Herbig disks as seen by ALMA
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Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H α
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ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)
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A giant planet shaping the disk around the very low-mass star CIDA 1
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Exploring the link between star and planet formation with Ariel
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COol Companions ON Ultrawide orbiTS (COCONUTS). III. A Very Red L6 Benchmark Brown Dwarf around a Young M5 Dwarf
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Disk Evolution Study through Imaging of Nearby Young Stars (DESTINYS): A Panchromatic View of DO Tau’s Complex Kilo-astronomical-unit Environment
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Single-dish 1-cm-band radio photometry of protoplanetary discs: few centimetre-sized dust grains?
Jane S Greaves and Brian MasonMonthly Notices of the Royal Astronomical Society 513 (3) 3180 (2022)
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Chemical Diversity in Protoplanetary Disks and Its Impact on the Formation History of Giant Planets
Elenia Pacetti, Diego Turrini, Eugenio Schisano, Sergio Molinari, Sergio Fonte, Romolo Politi, Patrick Hennebelle, Ralf Klessen, Leonardo Testi and Ugo LebreuillyThe Astrophysical Journal 937 (1) 36 (2022)
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Linking Atmospheric Chemistry of the Hot Jupiter HD 209458b to Its Formation Location through Infrared Transmission and Emission Spectra
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Underestimation of the dust mass in protoplanetary disks: Effects of disk structure and dust properties
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Importance of source structure on complex organics emission
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The CARMENES search for exoplanets around M dwarfs
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Modelling photoevaporation in planet forming discs
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Massive Compact Dust Disk with a Gap around CW Tau Revealed by ALMA Multiband Observations
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Evidence of a signature of planet formation processes from solar neutrino fluxes
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RV-detected planets around M dwarfs: Challenges for core accretion models
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The He I λ10830 Å line as a probe of winds and accretion in young stars in Lupus and Upper Scorpius
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The protoplanetary disk population in the ρ-Ophiuchi region L1688 and the time evolution of Class II YSOs
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Formation of Dust Clumps with Sub-Jupiter Mass and Cold Shadowed Region in Gravitationally Unstable Disk around Class 0/I Protostar in L1527 IRS
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Dynamical mass measurements of two protoplanetary discs
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