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--- examples_aswns_kepler [2022/08/16 21:55]
theoastro [A first Test]
+++ examples_aswns_kepler [2022/08/16 22:02] (current)
theoastro [Plotting your results]
@@ Line 65: / Line 65: @@
 The final results will be written in the file that you provided, by default this would be kepler.dat. The individual columns refer to:
-   * the central density
+     * the central density
-  * axial Omega
+    * axial Omega
-  * the corresponding error flag (0 means no error)
+    * the corresponding error flag (0 means no error)
-  * the gravitational mass in Msun
+    * the gravitational mass in Msun
-  * the baryonic mass in Msun
+    * the baryonic mass in Msun
-  * total stellar entropy,
+    * the proper mass
-  * the angular momentum
+    * total stellar entropy,
-   * the rotational energy
+    * the angular momentum
-   * the equatorial omega,
+    * the rotational energy
-   * the Keplerian Omega
+    * the equatorial omega,
-   *  the equatorial radius in Msun,
+    * the Keplerian Omega
+    *  the equatorial radius in Msun,
     * the equatorial radius in km
     *  radius at the pole in Msun
-     *  the disk mass
+    *  the disk mass
     * the derivative dm/drho
 ==== Plotting your results ====
+Based on the result in kepler.dat, you could check your results. One straight forward way would be to look at m(rho) and plot this with gnuplot, e.g.,
+gnuplot
+gnuplot> plot 'kepler.dat' u 1:4 w l
+which gives you the following plot of the gravitational mass as a function of the central density.
+{{aswns_kepler_simple.png}}

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