English

Rigidly rotating, incompressible spheroid-ring systems: new bifurcations, critical rotations and degenerate states

Solar and Stellar Astrophysics 2019-07-19 v1

Abstract

The equilibrium of incompressible spheroid-ring systems in rigid rotation is investigated by numerical means for a unity density contrast. A great diversity of binary configurations is obtained, with no limit neither in the mass ratio, nor in the orbital separation. We found only detached binaries, meaning that the end-point of the ϵ2\epsilon_2-sequence is the single binary state in strict contact, easily prone to mass-exchange. The solutions show a remarkable confinement in the rotation frequency-angular momentum diagram, with a total absence of equilibrium for Ω2/πGρ0.21\Omega^2/ \pi G \rho \gtrsim 0.21. A short band of degeneracy is present next to the one-ring sequence. We unveil a continuum of bifurcations all along the ascending side of the Maclaurin sequence for eccentricities of the ellipsoid less than 0.612\approx 0.612 and which involves a gradually expanding, initially massless loop.

Keywords

Cite

@article{arxiv.1907.08151,
  title  = {Rigidly rotating, incompressible spheroid-ring systems: new bifurcations, critical rotations and degenerate states},
  author = {B. Basillais and J. -M. Huré},
  journal= {arXiv preprint arXiv:1907.08151},
  year   = {2019}
}

Comments

Accepted for publication in MNRAS