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--- tests:discs:gc2014_spiralarms [2014/10/29 09:31] – sroca
+++ tests:discs:gc2014_spiralarms [2022/10/24 12:26] (current) – external edit 127.0.0.1
@@ Line 11: / Line 11: @@
 === Results ===
+Line of sight velocity of an axisymmetric distribution as function of galactic longitude:
+{{:tests:discs:vlos_helio_axisym.jpeg?200|}}
+{{:tests:discs:vlos_helio_axisym_in.jpeg?200|}}
+Residual l.o.s. velocity of an axisymetric distribution as function of galactic longitude:
+{{:tests:discs:vlos_res_axisym.jpeg?200|}}
+Substracted rotation curve:
+{{:tests:discs:rotcurv_axisym.pdf|}}
+-What we see is the velocity dispersion (no non-axisymmetric structures present in the model)
+-The asymmetry could be a consequence of the asymmetrical drift (it needs to be tested).
 === Data ===
@@ Line 59: / Line 76: @@
+https://drive.google.com/file/d/0B8sgZGL4aKpScGRKRnFSdXpyZDg/view?usp=sharing
@@ Line 80: / Line 97: @@
 -N-body spiral arms (Nd=3*10^6) / Unbarred Great Design spiral (Debatista14)
-In each row:  Id(1=?,2=?center), x(Kpc), y(Kpc), z(Kpc), vx(Km/s), vy(Km/s), vz(Km/s), ID2
+In each row:  Id(1=disk,2=bulge), x(Kpc), y(Kpc), z(Kpc), vx(Km/s), vy(Km/s), vz(Km/s), Mass (=1)
@@ Line 86: / Line 103: @@
 -Cartesian to equatorial + astrometric proper motions (Carmen)
+https://github.com/agabrown/PyGaia
 -Cartesian to observable (Abedi)