Instability, turbulence, and enhanced transport in accretion disks
SA Balbus, JF Hawley - Reviews of modern physics, 1998 - APS
Recent years have witnessed dramatic progress in our understanding of how turbulence
arises and transports angular momentum in astrophysical accretion disks. The key …
arises and transports angular momentum in astrophysical accretion disks. The key …
Circumbinary accretion: From binary stars to massive binary black holes
We review recent works on the dynamics of circumbinary accretion, including time variability,
angular momentum transfer between the disk and the binary, and the secular evolution of …
angular momentum transfer between the disk and the binary, and the secular evolution of …
[BOOK][B] Mathematical Topics in Fluid Mechanics: Volume 2: Compressible Models
PL Lions - 1996 - books.google.com
This series of books forms a unique and rigorous treatise on various mathematical aspects
of fluid mechanics models. These models consist of systems of nonlinear partial differential …
of fluid mechanics models. These models consist of systems of nonlinear partial differential …
Merger rate of primordial black-hole binaries
Primordial black holes (PBHs) have long been a candidate for the elusive dark matter (DM),
and remain poorly constrained in the∼ 20–100 M⊙ mass range. PBH binaries were …
and remain poorly constrained in the∼ 20–100 M⊙ mass range. PBH binaries were …
Orbital migration of the planetary companion of 51 Pegasi to its present location
DNC Lin, P Bodenheimer, DC Richardson - Nature, 1996 - nature.com
THE recent discovery1 and confirmation2 of a possible planetary companion orbiting the
solar-type star 51 Pegasi represent a breakthrough in the search for extrasolar planetary …
solar-type star 51 Pegasi represent a breakthrough in the search for extrasolar planetary …
Three-dimensional interaction between a planet and an isothermal gaseous disk. I. Corotation and Lindblad torques and planet migration
H Tanaka, T Takeuchi, WR Ward - The Astrophysical Journal, 2002 - iopscience.iop.org
Gravitational interaction between a planet and a three-dimensional isothermal gaseous disk
is studied. In the present paper we mainly examine the torque on a planet and the resultant …
is studied. In the present paper we mainly examine the torque on a planet and the resultant …
Nonlinear outcome of gravitational instability in cooling, gaseous disks
CF Gammie - The Astrophysical Journal, 2001 - iopscience.iop.org
Thin, Keplerian accretion disks generically become gravitationally unstable at large radii. I
investigate the nonlinear outcome of such instability in cool disks using razor-thin, local …
investigate the nonlinear outcome of such instability in cool disks using razor-thin, local …
Protoplanet migration by nebula tides
WR Ward - Icarus, 1997 - Elsevier
The tidal interaction of a protoplanet with a circumstellar gaseous disk results in mutual
angular momentum exchange that modifies both the disk and the orbit of the secondary …
angular momentum exchange that modifies both the disk and the orbit of the secondary …
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 …
Nine localized deviations from Keplerian rotation in the DSHARP circumstellar disks: kinematic evidence for protoplanets carving the gaps
We present evidence for localized deviations from Keplerian rotation, ie, velocity" kinks," in 8
of the 18 circumstellar disks observed by the DSHARP program: DoAr 25, Elias 2–27, GW …
of the 18 circumstellar disks observed by the DSHARP program: DoAr 25, Elias 2–27, GW …