Changes between Version 5 and Version 6 of u/lchamandy
- Timestamp:
- 08/07/19 14:37:26 (6 years ago)
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u/lchamandy
v5 v6 1 1 = Movies Made Using Common Envelope Simulation Data = 2 2 3 [https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I] 4 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1070C/abstract Paper II] 3 [https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I]\\ 4 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1070C/abstract Paper II]\\ 5 5 Paper 3: Chamandy+2019b (available soon) 6 6 … … 13 13 Movies 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. 14 14 15 '''Figure 1/Figure 2---face-on density :'''\\15 '''Figure 1/Figure 2---face-on density in units of g cm^-3^:'''\\ 16 16 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Figure1_density_face-on_zoomed_143/rho___sliceP2_faceon_lview_250o0Rsun_P1dir_left_1e-08_0o01_orangehot_143.gif Face-on density (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 17 17 … … 22 22 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Paper1/Figure1_density_face-on_zoomed_151/rho___sliceP2_faceon_lview_250.0Rsun_P1dir_left_1e-08_0.01_orangehot_151.gif Face-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 23 23 24 '''Figure 4 top panel---edge-on density :'''\\24 '''Figure 4 top panel---edge-on density in units of g cm^-3^:'''\\ 25 25 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Figure4_density_edge-on_zoomed_143/rho___sliceP2_edgeonthroughparticles_lview_250.0Rsun_P1dir_left_1e-08_0.01_orangehot_143.gif Edge-on density (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 26 26 … … 31 31 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Paper1/Figure4_density_edge-on_zoomed_151/rho___sliceP2_edgeonthroughparticles_lview_250.0Rsun_P1dir_left_1e-08_0.01_orangehot_151.gif Edge-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 32 32 33 '''Figure 4 bottom panel---edge-on density, zoomed in :'''\\33 '''Figure 4 bottom panel---edge-on density, zoomed in, in units of g cm^-3^:'''\\ 34 34 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Figure4_density_edge-on_zoomed_143/rho___sliceP2_edgeonthroughparticles_lview_30.0Rsun_P1dir_left_1e-06_0.01_Spectral_143.gif Edge-on density (zoomed in) (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 35 35 … … 40 40 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Paper1/Figure4_density_edge-on_zoomed_151/rho___sliceP2_edgeonthroughparticles_lview_30.0Rsun_P1dir_left_1e-06_0.01_Spectral_151.gif Edge-on density (zoomed in) (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 41 41 42 '''Figure 6---flow around companion :'''\\42 '''Figure 6---flow around companion, tangential velocity in rest frame of companion, corotating with particle orbit, normalized to Keplerian value (vectors show velocity):'''\\ 43 43 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Figure8_velocity_143/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_143.gif Tangential velocity with velocity vectors (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 44 44 … … 52 52 Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame. 53 53 54 '''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors arevelocity):'''\\54 '''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors show velocity):'''\\ 55 55 [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)]\\ 56 56 … … 59 59 [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)]\\ 60 60 61 '''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 arevelocity):'''\\61 '''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):'''\\ 62 62 [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)]\\ 63 63 … … 88 88 89 89 == Side-by-side comparison of Model A (left) and Model IB (right) from Paper 1 == 90 [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 ]\\91 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures4top_rho.gif Edge-on density ]\\92 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures4bottom_rho.gif Edge-on density , zoomed]\\93 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figure6.gif Tangential velocity ]\\94 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Temperature.gif Temperature ]\\95 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/c_s.gif Sound speed ]\\96 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Mach.gif Mach in lab frame]\\97 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Mach_corot_rel_2.gif Mach in frame corotating about secondary]\\90 [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 g cm^-3^]\\ 91 [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 g cm^-3^]\\ 92 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures4bottom_rho.gif Edge-on density in g cm^-3^, zoomed]\\ 93 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figure6.gif Tangential velocity, as above]\\ 94 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Temperature.gif Temperature, in K]\\ 95 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/c_s.gif Sound speed, in km s^-1^]\\ 96 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Mach.gif Mach number in lab frame]\\ 97 [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]\\ 98 98 99 99