Changes between Version 15 and Version 16 of u/lchamandy

Timestamp:

02/15/20 21:18:17 (5 years ago)

Author:

Luke

Comment:

—

u/lchamandy

@@ -3 +3 @@
 [https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I: Chamandy+2018 "Accretion in Common Envelope Evolution"]\\
 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1070C/abstract Paper II: Chamandy+2019a "Energy Budget and Core-Envelope Motion in Common Envelope Evolution"]\\
-[https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.3727C/abstract Paper III: Chamandy+2019b "How Drag Force Evolves in Global Common Envelope Simulations"]
+[https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.3727C/abstract Paper III: Chamandy+2019b "How Drag Force Evolves in Global Common Envelope Simulations"]\\
+Units on colorbars are CGS (except for in some cases where dimensionless units are used).
 
 == Density (zoomed in) in lab frame ==
@@ -12 +13 @@
 == Movies corresponding to figures in Paper III (for Model A and Models B and C of Paper III). Companion (particle 2) at center of frame, red giant core (particle 1) located on -y axis.
 
-'''Figure 6 first row---face-on force density (contours equal to values on colorbar, blue arrow shows velocity of particle 2 in rest frame of particle 1, black arrow shows net force on particle 2 in rest frame of particle 1):'''\\
+'''Figure 6 first row---face-on force density on particle 2 in rest frame of particle 1 in dyn/cm^3^ (contours equal to values on colorbar, blue arrow shows velocity of particle 2 in rest frame of particle 1, black arrow shows net force on particle 2 in rest frame of particle 1):'''\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/modFgas2phi_rel_1__Fgas2phi_rel_1_Fgas2phi_rel_1_sliceP2_faceon_lview_120Rsun_P1dir_bottom_1e-06_10_Spectral_Run143.gif Face-on force density (Model A: No subgrid accretion, M2 = 1 Msun)]\\
 
@@ -19 +20 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/modFgas2phi_rel_1__Fgas2phi_rel_1_Fgas2phi_rel_1_sliceP2_faceon_lview_120Rsun_P1dir_bottom_1e-06_10_Spectral_Run151.gif Face-on force density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
 
-'''Figure 5 second row---face-on density normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
+'''Figure 6 second row---face-on density normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/rho_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_1.0_1000.0_plasma_Run143.gif Face-on normalized density (Model A: No subgrid accretion, M2 = 1 Msun)]\\
 
@@ -26 +27 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/rho_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_1.0_1000.0_plasma_Run151.gif Face-on normalized density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
 
-'''Figure 5 third row---face-on Mach number in co-orbiting and co-rotating reference frame of particle 2:'''\\
+'''Figure 6 third row---face-on Mach number in co-orbiting and co-rotating reference frame of particle 2:'''\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Mach_corot_rel_2___sliceP2_faceon_lview_30Rsun_P1dir_bottom_0.1_10_RdBu_Run143.gif Face-on Mach number (Model A: No subgrid accretion, M2 = 1 Msun)]\\
 
@@ -33 +34 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Mach_corot_rel_2___sliceP2_faceon_lview_30Rsun_P1dir_bottom_0.1_10_RdBu_Run151.gif Face-on Mach number (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
 
-'''Figure 5 fourth row---face-on tangential velocity (with respect to particle 1) normalized to value calculated assuming a circular orbit at radius r=a(t) and density profile of initial envelope (assumed non-rotating). Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
+'''Figure 6 fourth row---face-on tangential velocity (with respect to particle 1) normalized to value calculated assuming a circular orbit at radius r=a(t) and density profile of initial envelope (assumed non-rotating). Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/v_rel_1_phi_corot_rel_2_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_-2_2_Spectral_Run143.gif Face-on normalized tangential velocity (Model A: No subgrid accretion, M2 = 1 Msun)]\\
 
@@ -40 +41 @@
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/v_rel_1_phi_corot_rel_2_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_-2_2_Spectral_Run151.gif Face-on normalized tangential velocity (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
 
-'''Figure 5 fifth row---face-on sound speed (with respect to particle 1) normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
+'''Figure 6 fifth row---face-on sound speed (with respect to particle 1) normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in co-orbiting and co-rotating rest frame of particle 2:'''\\
 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/c_s_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_0_8_caleblack_Run143.gif Face-on normalized sound speed (Model A: No subgrid accretion, M2 = 1 Msun)]\\