Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift [PDF]
Astrophysical Journal, 2018 Current models of (exo)planet formation often rely on a large influx of so-called “pebbles” from the outer disk into the planet formation region.
S. Krijt +3 more
semanticscholar +1 more source
Ionization and heating by X-rays and cosmic rays*
EPJ Web of Conferences, 2015 High-energy radiation from the central T Tauri and protostars plays an important role in shaping protoplanetary disks and influences their evolution. Such radiation, in particular X-rays and extreme-ultraviolet (EUV) radiation, is predominantly generated
Güdel Manuel
doaj +1 more source
The Astrophysical Journal, 2023 We present a three-dimensional, time-dependent MHD simulation of the short-term interaction between a protoplanetary disk and the stellar corona in a T Tauri system.
Ofer Cohen +6 more
doaj +1 more source
The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA Maps of Protoplanetary Disks in Terms of a Dust Model [PDF]
Astrophysical Journal, 2018 The Disk Substructures at High Angular Resolution Project (DSHARP) is the largest homogeneous high-resolution (∼0.″035, or ∼5 au) disk continuum imaging survey with the Atacama Large Millimeter/submillimeter Array (ALMA) so far. In the coming years, many
T. Birnstiel +11 more
semanticscholar +1 more source
Formation of giant planets around stars with various masses [PDF]
, 2006 We examine the predictions of the core accretion - gas capture model concerning the efficiency of planet formation around stars with various masses. First, we follow the evolution of gas and solids from the moment when all solids are in the form of small
Bodenheimer +32 more
core +2 more sources
A Survey of C2H, HCN, and C18O in Protoplanetary Disks [PDF]
Astrophysical Journal, 2019 Molecular lines observed toward protoplanetary disks carry information about physical and chemical processes associated with planet formation. We present ALMA Band 6 observations of C2H, HCN, and C18O in a sample of 14 disks spanning a range of ages ...
J. Bergner +5 more
semanticscholar +1 more source
Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet [PDF]
Astrophysical Journal, 2019 Dust growth is often neglected when building models of protoplanetary disks due to its complexity and computational expense. However, it does play a major role in shaping the evolution of protoplanetary dust and planet formation.
J. Dra̧żkowska +4 more
semanticscholar +1 more source
PAHs in protoplanetary disks: emission and X-ray destruction [PDF]
, 2012 We study the PAH emission from protoplanetary disks. First, we discuss the dependence of the PAH band ratios on the hardness of the absorbed photons and the temperature of the stars.
Acke +60 more
core +1 more source
Probing CO and N2 Snow Surfaces in Protoplanetary Disks with N2H+ Emission [PDF]
Astrophysical Journal, 2019 Snowlines of major volatiles regulate the gas and solid C/N/O ratios in the planet-forming midplanes of protoplanetary disks. Snow surfaces are the 2D extensions of snowlines in the outer disk regions, where radiative heating results in an increasing ...
C. Qi +8 more
semanticscholar +1 more source
Centimeter-sized Grains in the Compact Dust Ring around Very-low-mass Star CIDA 1
The Astronomical Journal, 2023 We examined the grain size in the dust ring encircling the 0.19 M _☉ T Tauri star CIDA 1 using the Karl G. Jansky Very Large Array at multiple centimeter wavelengths, with a spatial resolution of 0.″2–0.″9. We detected distinct partial-ring structures at
Jun Hashimoto +5 more
doaj +1 more source