Results 91 to 100 of about 14,974 (190)

A Lagrangian Integrator for Planetary Accretion and Dynamics (LIPAD)

, 2012
We presented the first particle based, Lagrangian code that can follow the collisional/accretional/dynamical evolution of a large number of km-sized planetesimals through the entire growth process to become planets.
Binney, Bromley, Chambers, Duncan, Edward Thommes, Hahn, Harold F. Levison, Hayashi, Ida, Kenyon, Kenyon, Kenyon, Levison, Levison, Lissauer, Martin J. Duncan, Minton, Robertson, Skeel, Spitzer, Trubnikov   +20 more
core   +1 more source

Oligarchic Growth of Protoplanets in Planetesimal Rings

The Astrophysical Journal
In the standard planet formation scenario, planetesimals are assumed to form throughout the protoplanetary disk and to be smoothly distributed in the radial direction except for the snowline.
Yuki Kambara, Eiichiro Kokubo
doaj   +1 more source

Linking planetesimal and dust content in protoplanetary disks via a local toy model [PDF]

, 2019
Konstantin Gerbig, Christian T. Lenz, Hubert Klahr   +2 more
openalex   +1 more source

Planetesimal formation in turbulent circumstellar disks [PDF]

, 2010
David Robert Kirsh, Ralph E. Pudritz
openalex   +1 more source

An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion [PDF]

, 2023
Wladimir Lyra, Anders Johansen, Manuel H. Cañas, Chao‐Chin Yang   +3 more
openalex   +1 more source

Argon in β Pictoris–Entrapment and Release of Volatile in Disks

The Astrophysical Journal
Chemical compositions of planets reveal much about their formation environments. Such information is well sought-after in studies of solar system bodies and extrasolar ones.
Yanqin Wu, Kadin Worthen, Alexis Brandeker, Christine Chen   +3 more
doaj   +1 more source

Insights into Planet Formation from Debris Disks: I. The Solar System as an Archetype for Planetesimal Evolution [PDF]

, 2016
Brenda C. Matthews, J. J. Kavelaars
openalex   +1 more source

Rapid planetesimal formation in the inner protoplanetary disk [PDF]

, 2014
Joanna Dra̧żkowska, F. Windmark⋆, Satoshi Okuzumi   +2 more
openalex   +1 more source

Observing planetesimal formation under streaming instability in the rings of HD 163296 [PDF]

, 2023
Francesco Zagaria, C. J. Clarke, Richard A Booth, Stefano Facchini, Giovanni Rosotti   +4 more
openalex   +1 more source

Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall

The Astrophysical Journal
There is growing evidence that planet formation begins early, within the ≲1 Myr Class 0/I phase, when infall dominates disk dynamics. Our goal is to determine if Class 0/I disks reach the conditions needed to form planetesimals (∼100 km planet building ...
Daniel Carrera, Abigail Davenport, Jacob B. Simon, Hans Baehr, Til Birnstiel, Cassandra Hall, David Rea, Sebastian Markus Stammler   +7 more
doaj   +1 more source