Sentence examples for binary axis from inspiring English sources

Both versions have two basic output options: one provides values of a set of various quantities (such as the Lagrange points along the binary axis, and area and volume of the Roche lobe); the second provides (R(theta,phi)), the distance from the stellar center to the stellar surface for any specified polar angle.

For the binary semimajor axis we obtain: delta a = frac{2}{m^{2}} a^{2} delta E. (13) Here a is the semimajor axis from the Brutus solution.

The binary semimajor axis and binding energy are related quantities.

The errors are given for the dissolution time (left column), binary semimajor axis (middle column) and eccentricity (right column).

The bias in the left column for the binary semimajor axis is caused by solutions which grossly violate energy conservation.

Distributions are given for the escaper speed (top left) and kinetic energy (top right), binary semimajor axis (middle left), binding energy (middle right) and binary eccentricity (bottom).

We compare distributions of dissolution time (top left), escaper speed (top right), binary semimajor axis (bottom left) and binary eccentricity (bottom right)).

In the panel showing the data for the binary semimajor axis, the distributions of the cold systems become significantly different for (eta> 2^{-6}).

In Figure 14, we replot the average error in the binary semimajor axis as a function of the time-step parameter.

For the binary semimajor axis however, the data representing the cold collapse simulations also seem to be systematically biased for small time-steps, in the sense that Hermite makes fewer tight binaries.

We show distributions of the positive (solid, black) and negative (dashed, red) errors in the total energy (top row), total angular momentum (second row), escaper velocity (third row), binary semimajor axis fourth row) and eccentricity (bottom row).