Changes between Version 11 and Version 12 of u/lchamandy


Ignore:
Timestamp:
08/14/19 22:16:00 (6 years ago)
Author:
Luke
Comment:

—

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  • u/lchamandy

    v11 v12  
    1010[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/rho2D_faceon_zoom_151.gif Face-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    1111
    12 == Movies corresponding to figures in Paper I ==
     12== 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.
     13
     14'''Figure 5 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):'''\\
     15[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)]\\
     16
     17[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/modFgas2phi_rel_1__Fgas2phi_rel_1_Fgas2phi_rel_1_sliceP2_faceon_lview_120Rsun_P1dir_bottom_1e-06_10_Spectral_Run149.gif Face-on force density (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     18
     19[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)]\\
     20
     21'''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:'''\\
     22[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)]\\
     23
     24[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/rho_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_1.0_1000.0_plasma_Run149.gif Face-on normalized density (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     25
     26[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)]\\
     27
     28'''Figure 5 third row---face-on Mach number in co-orbiting and co-rotating reference frame of particle 2:'''\\
     29[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)]\\
     30
     31[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/Mach_corot_rel_2___sliceP2_faceon_lview_30Rsun_P1dir_bottom_0.1_10_RdBu_Run149.gif Face-on Mach number (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     32
     33[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)]\\
     34
     35'''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:'''\\
     36[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)]\\
     37
     38[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/v_rel_1_phi_corot_rel_2_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_-2_2_Spectral_Run149.gif Face-on normalized tangential velocity (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     39
     40[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)]\\
     41
     42'''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:'''\\
     43[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)]\\
     44
     45[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/c_s_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_0_8_caleblack_Run149.gif Face-on normalized sound speed (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     46
     47[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 IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
     48
     49== Movies corresponding to figures in Paper II (for Model A and Models B and C of Paper III)==
     50Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame.
     51
     52'''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors show velocity):'''\\
     53[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_143.gif Face-on normalized energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
     54
     55[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_149.gif Face-on normalized energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     56
     57[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_151.gif Face-on normalized energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
     58
     59'''Figure 3 second from top row---face-on normalized gas kinetic energy (magenta means thermal energy dominates, green means bulk KE dominates, yellow is density contours, vectors show velocity):'''\\
     60[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_143.gif Face-on normalized kinetic energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
     61
     62[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_149.gif Face-on normalized kinetic energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     63
     64[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_151.gif Face-on normalized kinetic energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
     65
     66== Movies corresponding to figures in Paper I (for Model A and Models B and C of Paper III and Model B of Paper I)==
    1367Movies are in the reference '''frame corotating about the secondary''' with the instantaneous orbital angular speed of the particles, and with the secondary at the center.
    1468
    … …  
    80134[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Mach_corot_rel_2.gif Mach number in frame corotating about secondary]\\
    81135
    82 == Movies corresponding to figures in Paper II ==
    83 Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame.
    84 
    85 '''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors show velocity):'''\\
    86 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_143.gif Face-on normalized energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
    87 
    88 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_149.gif Face-on normalized energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
    89 
    90 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_151.gif Face-on normalized energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    91 
    92 '''Figure 3 second from top row---face-on normalized gas kinetic energy (magenta means thermal energy dominates, green means bulk KE dominates, yellow is density contours, vectors show velocity):'''\\
    93 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_143.gif Face-on normalized kinetic energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
    94 
    95 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_149.gif Face-on normalized kinetic energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
    96 
    97 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_151.gif Face-on normalized kinetic energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    98 
    99 == Movies corresponding to figures in Paper III ==
    100 
    101 '''Coming soon'''