Results 71 to 80 of about 3,153 (136)

Empirical Stability Criteria for 3D Hierarchical Triple Systems. I. Circumbinary Planets

open access: yesThe Astronomical Journal
In this work we revisit the problem of the dynamical stability of hierarchical triple systems with applications to circumbinary planetary orbits. We derive critical semimajor axes based on simulating and analyzing the dynamical behavior of 3 × 10 ^8 ...
Nikolaos Georgakarakos   +3 more
doaj   +1 more source

On the formation and migration of giant planets in circumbinary discs [PDF]

open access: yesAstronomy & Astrophysics, 2008
We present the results of hydrodynamic simulations of the formation and subsequent orbital evolution of giant planets embedded in a circumbinary disc. We assume that a 20 earth masses core has migrated to the edge of the inner cavity formed by the binary where it remains trapped by corotation torques.
Arnaud Pierens, Richard P. Nelson
openaire   +3 more sources

Kozai-Lidov cycles towards the limit of circumbinary planets

open access: yes, 2015
In this paper we answer a simple question: can a misaligned circumbinary planet induce Kozai-Lidov cycles on an inner stellar binary? We use known analytic equations to analyse the behaviour of the Kozai-Lidov effect as the outer mass is made small.
Martin, David V.   +1 more
core   +1 more source

Circumbinary planets – why they are so likely to transit [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Transits on single stars are rare. The probability rarely exceeds a few per cent. Furthermore, this probability rapidly approaches zero at increasing orbital period. Therefore transit surveys have been predominantly limited to the inner parts of exoplanetary systems. Here we demonstrate how circumbinary planets allow us to beat these unfavourable odds.
Martin, David V.   +1 more
openaire   +4 more sources

Planetary Rhythms: Synchronous Circulation on Variably Irradiated Asynchronous Planets

open access: yesThe Astrophysical Journal
Tidal locking of planets to their host stars results in an atmospheric circulation with a hotspot fixed to the frame of reference of the planet. On the other hand, asynchronously rotating planets feature moving hotspots either lagging or leading the ...
Deepayan Banik
doaj   +1 more source

Evolution of circumbinary planets around eccentric binaries: The case of Kepler-34

open access: yes, 2015
The existence of planets orbiting a central binary star system immediately raises questions regarding their formation and dynamical evolution. Recent discoveries of circumbinary planets by the Kepler space telescope has shown that some of these planets ...
Haghighipour, Nader, Kley, Wilhelm
core   +1 more source

Sites of Planet Formation in Binary Systems. I. Evidence for Disk−Orbit Alignment in the Close Binary FO Tau

open access: yesThe Astronomical Journal
Close binary systems present challenges to planet formation. As binary separations decrease, so do the occurrence rates of protoplanetary disks in young systems and planets in mature systems.
Benjamin M. Tofflemire   +10 more
doaj   +1 more source

Young Binary Stars and Associated Disks [PDF]

open access: yes, 1999
The typical product of the star formation process is a binary star. Binaries have provided the first dynamical measures of the masses of pre-main-sequence (PMS) stars, providing support for the calibrations of PMS evolutionary tracks.
Ghez, Andrea M.   +3 more
core   +2 more sources

Regions of Dynamical Stability for Discs and Planets in Binary Stars of the Solar Neighborhood

open access: yes, 2012
Using the results of Pichardo \et (2005,2008), we determine regions of dynamical stability where planets (or discs in general) could survive in stable orbits around binary stellar systems.
Aguilar, Luis   +2 more
core   +1 more source

Dynamics of Circumstellar Disks III: The case of GG Tau A

open access: yes, 2016
(abridged) We present 2-dimensional hydrodynamic simulations using the Smoothed Particle Hydrodynamic (SPH) code, VINE, to model a self-gravitating binary system similar to the GG Tau A system.
Marzari, F., Nelson, Andrew F.
core   +1 more source

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