Results 21 to 30 of about 3,808,369 (275)

A colorful view of planet formation:A multi-wavelength study of planet-disk interactions [PDF]

open access: yes, 2021
The broad variety of planets and planetary systems discovered in the last couple of decades around other stars has taught us that these can be, and more often than not tend to be, very different from our own.
Muro Arena, G.A.
core   +5 more sources

Planet–Disk Interaction in Disks with Cooling: Basic Theory [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract Gravitational coupling between young planets and their parent disks is often explored using numerical simulations, which typically treat the disk thermodynamics in a highly simplified manner. In particular, many studies adopt the locally isothermal approximation, in which the disk temperature is a fixed function of the ...
Ryan Miranda, Roman R. Rafikov
openaire   +2 more sources

Constraining the gas distribution in the PDS 70 disk as a method to assess the effect of planet-disk interactions [PDF]

open access: yes, 2023
Embedded planets are potentially the cause of substructures like gaps and cavities observed in several protoplanetary disks. Thus, the substructures observed in the continuum and in line emission encode information about the presence of planets in the ...
Law, C.   +25 more
core   +1 more source

Planet-Disk Interactions

open access: yes, 2022
Planet-disk interactions, where an embedded massive body interacts gravitationally with the protoplanetary disk it was formed in, can play an important role in reshaping both the disk and the orbit of the planet. Spiral density waves are launched into the disk by the planet, which, if they are strong enough, can lead to the formation of a gap.
Paardekooper, Sijme-Jan   +6 more
openaire   +2 more sources

Planet-Disk Interaction revisited [PDF]

open access: yesEPJ Web of Conferences, 2013
We present results on our investigations of planet–disk interaction in protoplanetary disks. For the hydrodynamic simulations we use a second order semi–discrete total variation diminishing (TVD) scheme for systems of hyperbolic conservation laws on curvilinear grids.
Illenseer T. F.   +2 more
openaire   +2 more sources

Excitation of Planetary Obliquities through Planet–Disk Interactions [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract The tilt of a planet’s spin axis off its orbital axis (“obliquity”) is a basic physical characteristic that plays a central role in determining the planet’s global circulation and energy redistribution. Moreover, recent studies have also highlighted the importance of obliquities in sculpting not only the physical features of ...
Sarah Millholland, Konstantin Batygin
openaire   +3 more sources

SO and SiS Emission Tracing an Embedded Planet and Compact 12CO and 13CO Counterparts in the HD 169142 Disk

open access: yesThe Astrophysical Journal Letters, 2023
Planets form in dusty, gas-rich disks around young stars, while at the same time, the planet formation process alters the physical and chemical structure of the disk itself. Embedded planets will locally heat the disk and sublimate volatile-rich ices, or
Charles J. Law   +2 more
doaj   +1 more source

On the number of particles in N-body simulations of planet–disk interaction [PDF]

open access: yesPlanetary and Space Science, 2007
Abstract In this paper we present a new mixed-variables symplectic tree code for planetesimal dynamics, which allows to use a very large number of particles in numerical simulations of planet–disk interaction. Furthermore, we discuss how a wrong election of the number of particles to model a planetesimal disk, in order to carry out realistic ...
Brunini, Adrián   +3 more
openaire   +3 more sources

Planet-Disk interaction in 3D: the importance of buoyancy waves [PDF]

open access: yesThe Astrophysical Journal, 2012
4 pages, 4 figures, Accepted by ApJ ...
Zhu, Zhaohuan   +2 more
openaire   +3 more sources

The Effect of Convective Overstability on Planet Disk Interactions [PDF]

open access: yesProceedings of the International Astronomical Union, 2015
AbstractWe run global two dimensional hydrodynamical simulations, using the PLUTO code and the planet-disk model of Uribe et al. 2011, to investigate the effect of the convective overstability (CO) on planet-disk interactions. First, we study the long-term evolution of planet-induced vortices. We found that the CO leads to smoother planetary gap edges,
Hubert Klahr, Aiara Lobo Gomes
openaire   +1 more source

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