Observations of protoplanetary disk structures
SM Andrews - Annual Review of Astronomy and Astrophysics, 2020 - annualreviews.org
The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …
and planet formation. Their structures, meaning the spatial variations of the disk physical …
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 …
Formation of planetary systems by pebble accretion and migration-How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode
M Lambrechts, A Morbidelli, SA Jacobson… - Astronomy & …, 2019 - aanda.org
Super-Earths–planets with sizes between the Earth and Neptune–are found in tighter orbits
than that of the Earth around more than one third of main sequence stars. It has been …
than that of the Earth around more than one third of main sequence stars. It has been …
The radial distribution of dust particles in the HL Tau disk from ALMA and VLA observations
C Carrasco-González, A Sierra, M Flock… - The Astrophysical …, 2019 - iopscience.iop.org
Understanding planet formation requires one to discern how dust grows in protoplanetary
disks. An important parameter to measure in disks is the maximum dust grain size present …
disks. An important parameter to measure in disks is the maximum dust grain size present …
Formation of planetary systems by pebble accretion and migration: growth of gas giants
Giant planets migrate though the protoplanetary disc as they grow their solid core and attract
their gaseous envelope. Previously, we have studied the growth and migration of an isolated …
their gaseous envelope. Previously, we have studied the growth and migration of an isolated …
[HTML][HTML] Shadows and spirals in the protoplanetary disk HD 100453
M Benisty, T Stolker, A Pohl, J De Boer, G Lesur… - Astronomy & …, 2017 - aanda.org
Context. Understanding the diversity of planets requires studying the morphology and
physical conditions in the protoplanetary disks in which they form. Aims. We aim to study the …
physical conditions in the protoplanetary disks in which they form. Aims. We aim to study the …
Isotopic evolution of the protoplanetary disk and the building blocks of Earth and the Moon
Nucleosynthetic isotope variability among Solar System objects is often used to probe the
genetic relationship between meteorite groups and the rocky planets (Mercury, Venus, Earth …
genetic relationship between meteorite groups and the rocky planets (Mercury, Venus, Earth …
Formation of planetary systems by pebble accretion and migration-Hot super-Earth systems from breaking compact resonant chains
At least 30% of main sequence stars host planets with sizes of between 1 and 4 Earth radii
and orbital periods of less than 100 days. We use N-body simulations including a model for …
and orbital periods of less than 100 days. We use N-body simulations including a model for …
Early formation of planetary building blocks inferred from Pb isotopic ages of chondrules
The most abundant components of primitive meteorites (chondrites) are millimeter-sized
glassy spherical chondrules formed by transient melting events in the solar protoplanetary …
glassy spherical chondrules formed by transient melting events in the solar protoplanetary …
Multiple disk gaps and rings generated by a single Super-Earth
We investigate the observational signatures of super-Earths (ie, planets with Earth-to-
Neptune mass), which are the most common type of exoplanet discovered to date, in their …
Neptune mass), which are the most common type of exoplanet discovered to date, in their …