x(n) — y(°) + Q(X^,X^)=0 (3.11) and this system is typically nonlinear and has therefore to be solved itera- tively, e.g., by a Newton-Raphson iteration for the variables X^ at the new time level. Usually the time step is not restricted ...
Galactic Astronomy: Structure and Kinematics
This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications.
... MkT/V, (70.1) p = ptotal = pet P*=(WKTIV) +%asT“, (70.2) and define - o, EP”/ps. (70.3) The total internal energy in the volume is & = }MkT+ asT"V, (70.4) hence the specific internal energy per unit mass is =#RT+(asT“/p). (70.5) To ...
The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the ...
The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the ...