Planet-disk interaction and orbital evolution
W Kley, RP Nelson - Annual Review of Astronomy and …, 2012 - annualreviews.org
As planets form and grow within gaseous protoplanetary disks, the mutual gravitational
interaction between the disk and planet leads to the exchange of angular momentum and …
interaction between the disk and planet leads to the exchange of angular momentum and …
A new class of accurate, mesh-free hydrodynamic simulation methods
PF Hopkins - Monthly Notices of the Royal Astronomical Society, 2015 - academic.oup.com
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
Hydrodynamics of circumbinary accretion: angular momentum transfer and binary orbital evolution
We carry out 2D viscous hydrodynamical simulations of circumbinary accretion using the
moving-mesh code AREPO. We self-consistently compute the accretion flow over a wide …
moving-mesh code AREPO. We self-consistently compute the accretion flow over a wide …
The Ophiuchus DIsc Survey Employing ALMA (ODISEA)–III. The evolution of substructures in massive discs at 3–5 au resolution
LA Cieza, C González-Ruilova, AS Hales… - Monthly Notices of …, 2021 - academic.oup.com
We present 1.3 mm continuum ALMA long-baseline observations at 3–5 au resolution of 10
of the brightest discs from the Ophiuchus DIsc Survey Employing ALMA (ODISEA) project …
of the brightest discs from the Ophiuchus DIsc Survey Employing ALMA (ODISEA) project …
Radial migration of gap-opening planets in protoplanetary disks. I. The case of a single planet
KD Kanagawa, H Tanaka… - The Astrophysical …, 2018 - iopscience.iop.org
A large planet orbiting a star in a protoplanetary disk opens a density gap along its orbit due
to the strong disk–planet interaction and migrates with the gap in the disk. It is expected that …
to the strong disk–planet interaction and migrates with the gap in the disk. It is expected that …
How to model supernovae in simulations of star and galaxy formation
PF Hopkins, A Wetzel, D Kereš… - Monthly Notices of …, 2018 - academic.oup.com
We study the implementation of mechanical feedback from supernovae (SNe) and stellar
mass loss in galaxy simulations, within the Feedback In Realistic Environments (FIRE) …
mass loss in galaxy simulations, within the Feedback In Realistic Environments (FIRE) …
[HTML][HTML] On planet formation in HL Tau
G Dipierro, D Price, G Laibe, K Hirsh… - Monthly Notices of …, 2015 - academic.oup.com
We explain the axisymmetric gaps seen in recent long-baseline observations of the HL Tau
protoplanetary disc with the Atacama Large Millimetre/Submillimetre Array (ALMA) as being …
protoplanetary disc with the Atacama Large Millimetre/Submillimetre Array (ALMA) as being …
Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
We present Phantom, a fast, parallel, modular, and low-memory smoothed particle
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
Anisotropic infall and substructure formation in embedded disks
A Kuznetsova, J Bae, L Hartmann… - The Astrophysical …, 2022 - iopscience.iop.org
The filamentary nature of accretion streams found around embedded sources suggests that
protostellar disks experience heterogenous infall from the star-forming environment …
protostellar disks experience heterogenous infall from the star-forming environment …
A torque formula for non-isothermal type I planetary migration–I. Unsaturated horseshoe drag
SJ Paardekooper, C Baruteau, A Crida… - Monthly Notices of the …, 2010 - academic.oup.com
We study the torque on low-mass planets embedded in protoplanetary discs in the two-
dimensional approximation, incorporating non-isothermal effects. We couple linear …
dimensional approximation, incorporating non-isothermal effects. We couple linear …