Relative velocities among accreting planetesimals in binary systems: The circumprimary case
- Thébault, P.
- Marzari, F.
- Scholl, H.
DOIAbstract
Icarus, 183, pp. 193-206, http://dx.doi.org./10.1016/j.icarus..01.022International audienc
Icarus, 183, pp. 193-206, http://dx.doi.org./10.1016/j.icarus..01.022International audienc
International audienceWe present an analytical framework that accurately describes the motion of co-...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
The radial velocities of WY Velorum do not seem to show variations with time. If symbiotic stars are...
Icarus, 183, pp. 193-206, http://dx.doi.org./10.1016/j.icarus..01.022International audienc
Monthly Notices of the Royal Astronomical Society, 380, pp. 1119-1126, http://dx.doi.org./10.1111/j....
The extent to which planetesimal accretion is affected by the perturbing presence of a companion sta...
One of the major problems of planet formation in close binary systems, such as α Centauri AB, is the...
Planetesimal accretion in close binary systems is a complex process for the gravitational perturbati...
Aims: We explore planet formation in binary systems around the central star where the protoplanetary...
Observations of extrasolar planets reveal that planets can be found in close binary systems, where t...
Icarus, 188, pp. 522-534, http://dx.doi.org./10.1016/j.icarus.2006.12.006International audienc
Context. A large fraction of stars, including young T Tauri stars, are observed to be memb...
We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stir...
Context. The secular dynamics of small planetesimals in tight binary systems play a fundamental role...
We expand notes on Keplerian orbits of binary stars and derive equations of motion for radial veloci...
International audienceWe present an analytical framework that accurately describes the motion of co-...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
The radial velocities of WY Velorum do not seem to show variations with time. If symbiotic stars are...
Icarus, 183, pp. 193-206, http://dx.doi.org./10.1016/j.icarus..01.022International audienc
Monthly Notices of the Royal Astronomical Society, 380, pp. 1119-1126, http://dx.doi.org./10.1111/j....
The extent to which planetesimal accretion is affected by the perturbing presence of a companion sta...
One of the major problems of planet formation in close binary systems, such as α Centauri AB, is the...
Planetesimal accretion in close binary systems is a complex process for the gravitational perturbati...
Aims: We explore planet formation in binary systems around the central star where the protoplanetary...
Observations of extrasolar planets reveal that planets can be found in close binary systems, where t...
Icarus, 188, pp. 522-534, http://dx.doi.org./10.1016/j.icarus.2006.12.006International audienc
Context. A large fraction of stars, including young T Tauri stars, are observed to be memb...
We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stir...
Context. The secular dynamics of small planetesimals in tight binary systems play a fundamental role...
We expand notes on Keplerian orbits of binary stars and derive equations of motion for radial veloci...
International audienceWe present an analytical framework that accurately describes the motion of co-...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
The radial velocities of WY Velorum do not seem to show variations with time. If symbiotic stars are...
Add to ORKG