Changes between Version 9 and Version 10 of u/lchamandy

Timestamp:

08/08/19 13:03:32 (6 years ago)

Author:

Luke

Comment:

—

u/lchamandy

@@ -1 @@
-= Movies Made Using Common Envelope Simulation Data =
+= Movies Made Using Common Envelope Simulation Output =
 The relevant references for these movies are:\\ 
 [https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I: Chamandy+2018 "Accretion in Common Envelope Evolution"]\\
@@ -49 +49 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Paper1/Figure8_velocity_151/v_phi_over_v_Kepler_corot_rel_2_vVec_corot_rel_2_v_phi_over_v_Kepler_corot_rel_2_sliceP2_faceon_lview_30.0Rsun_P1dir_left_-1_0.5_rainbow_151.gif Tangential velocity with velocity vectors (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
 
-=== Extra Movies ===
+'''Extra Movies'''
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Temperature/Temperature___sliceP2_faceon_lview_250.0Rsun_P1dir_left_1000.0_10000000.0_viridis_143.gif Temperature (Model A: No subgrid accretion, M2 = 1 Msun)]\\
 
@@ -70 +70 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Damp132/Paper1/Mach/Mach_corot_rel_2___sliceP2_faceon_lview_250.0Rsun_P1dir_left_0.01_100_difference_132.gif Mach, frame corotating about secondary (Model IB: Subgrid accretion, M2 = 1 Msun)]\\
 
-=== Side-by-side comparison of Model A (left) and Model IB (right) from Paper I ===
+'''Side-by-side comparison of Model A (left) and Model IB (right) from Paper I'''
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures1-2_rho.gif Face-on density in cgs]\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures4top_rho.gif Edge-on density in cgs]\\