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Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-driven Growth of LIGO Binary Black Holes

  • Authors: Soumi De, Morgan MacLeod, Rosa Wallace Everson, Andrea Antoni, Ilya Mandel, and Enrico Ramirez-Ruiz

2020 The Astrophysical Journal 897 130.

  • Provider: AAS Journals

Caption: Figure 6.

Slices of density in units of ﹩{\rho }_{\infty }﹩ for the simulation suite (Γs, γ) = (4/3, 4/3) (left panels) and for the simulation suite (Γs, γ) = (5/3, 5/3) (right panels) through the orbital (xy) plane, for a fixed upstream Mach number ﹩{{ \mathcal M }}_{\infty }﹩ and varying ratio qr. The simulations for each γ use ﹩{{ \mathcal M }}_{\infty }=1.69﹩ and qr = 0.1 (top) and 0.33 (bottom). The slices compare the state of the flow at simulation time ﹩t=30{R}_{{\rm{a}}}/{v}_{\infty }﹩. The panels show the dependence of the flow pattern around the embedded companion object in a specific region of the envelope on the binary mass ratio.

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