Image Details
Caption: Figure 4.
Value of
f(ξ = 0, χ) as a function of χ—the fraction of
passing through the orbit of the secondary. Different curves correspond to different values of the power-law parameters
d and
p indicated in the figure: dotted lines correspond to the gas pressure-dominated case with κ = κ
es, and solid lines correspond to the gas pressure-dominated case with κ = κ
ff. Knowledge of
f(ξ = 0) permits a computation of the torque acting on the central binary for an arbitrary value of the "accretion fraction"
χ.
© 2013. The American Astronomical Society. All rights reserved.