Planet formation—Observational constraints, physical processes, and compositional patterns
C Mordasini, R Burn - Reviews in Mineralogy and …, 2024 - pubs.geoscienceworld.org
A general theory of planet formation has been a topic of intense study over many years. The
interest in such a theory emerges naturally from asking the question of where our planet …
interest in such a theory emerges naturally from asking the question of where our planet …
A tale of planet formation: from dust to planets
The characterization of exoplanets and their birth protoplanetary disks has enormously
advanced in the last decade. Benefitting from that, our global understanding of the planet …
advanced in the last decade. Benefitting from that, our global understanding of the planet …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …
classical planet formation theory, developed when the only known planetary system was our …
On the diversity of asymmetries in gapped protoplanetary disks
Protoplanetary disks with large inner dust cavities are thought to host massive planetary or
substellar companions. These disks show asymmetries and rings in the millimeter …
substellar companions. These disks show asymmetries and rings in the millimeter …
How to make giant planets via pebble accretion
S Savvidou, B Bitsch - Astronomy & Astrophysics, 2023 - aanda.org
Planet formation is directly linked to the birthing environment that protoplanetary disks
provide. The disk properties determine whether a giant planet will form and how it evolves …
provide. The disk properties determine whether a giant planet will form and how it evolves …
Dust Hot Spots at 10 au Scales around the Class 0 Binary IRAS 16293–2422 A: A Departure from the Passive Irradiation Model
Characterizing the physical conditions at disk scales in class 0 sources is crucial for
constraining the protostellar accretion process and the initial conditions for planet formation …
constraining the protostellar accretion process and the initial conditions for planet formation …
Constraints on the dust size distributions in the HD 163296 disk from the difference of the apparent dust ring widths between two ALMA Bands
The dust size in protoplanetary disks is a crucial parameter for understanding planet
formation, while the observational constraints on dust size distribution have large …
formation, while the observational constraints on dust size distribution have large …
Toward a population synthesis of disks and planets-II. Confronting disk models and observations at the population level
A Emsenhuber, R Burn, J Weder, K Monsch… - Astronomy & …, 2023 - aanda.org
Aims. We want to find the distribution of initial conditions that best reproduces disc
observations at the population level. Methods. We first ran a parameter study using a 1D …
observations at the population level. Methods. We first ran a parameter study using a 1D …
How dust fragmentation may be beneficial to planetary growth by pebble accretion
J Drążkowska, SM Stammler, T Birnstiel - Astronomy & Astrophysics, 2021 - aanda.org
Context. Pebble accretion is an emerging paradigm for the fast growth of planetary cores.
Pebble flux and pebble sizes are the key parameters used in the pebble accretion models …
Pebble flux and pebble sizes are the key parameters used in the pebble accretion models …
Gravitational Instability, Spiral Substructure, and Modest Grain Growth in a Typical Protostellar Disk: Modeling Multiwavelength Dust Continuum Observations of …
Embedded class 0/I protostellar disks represent the initial condition for planet formation. This
calls for a better understanding of their bulk properties and the dust grains within them. We …
calls for a better understanding of their bulk properties and the dust grains within them. We …