Changes between Version 15 and Version 16 of u/lchamandy
 Timestamp:
 02/15/20 21:18:17 (15 months ago)
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u/lchamandy
v15 v16 3 3 [https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I: Chamandy+2018 "Accretion in Common Envelope Evolution"]\\ 4 4 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1070C/abstract Paper II: Chamandy+2019a "Energy Budget and CoreEnvelope Motion in Common Envelope Evolution"]\\ 5 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.3727C/abstract Paper III: Chamandy+2019b "How Drag Force Evolves in Global Common Envelope Simulations"] 5 [https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.3727C/abstract Paper III: Chamandy+2019b "How Drag Force Evolves in Global Common Envelope Simulations"]\\ 6 Units on colorbars are CGS (except for in some cases where dimensionless units are used). 6 7 7 8 == 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. 13 14 14 '''Figure 6 first rowfaceon 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 '''Figure 6 first rowfaceon 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):'''\\ 15 16 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run143/modFgas2phi_rel_1__Fgas2phi_rel_1_Fgas2phi_rel_1_sliceP2_faceon_lview_120Rsun_P1dir_bottom_1e06_10_Spectral_Run143.gif Faceon force density (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 16 17 … … 19 20 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run151/modFgas2phi_rel_1__Fgas2phi_rel_1_Fgas2phi_rel_1_sliceP2_faceon_lview_120Rsun_P1dir_bottom_1e06_10_Spectral_Run151.gif Faceon force density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 20 21 21 '''Figure 5second rowfaceon density normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in coorbiting and corotating rest frame of particle 2:'''\\22 '''Figure 6 second rowfaceon density normalized to value at radius r=a(t) of initial envelope profile. Vectors show velocity field projected in orbital plane in coorbiting and corotating rest frame of particle 2:'''\\ 22 23 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run143/rho_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_1.0_1000.0_plasma_Run143.gif Faceon normalized density (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 23 24 … … 26 27 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run151/rho_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_1.0_1000.0_plasma_Run151.gif Faceon normalized density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 27 28 28 '''Figure 5third rowfaceon Mach number in coorbiting and corotating reference frame of particle 2:'''\\29 '''Figure 6 third rowfaceon Mach number in coorbiting and corotating reference frame of particle 2:'''\\ 29 30 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run143/Mach_corot_rel_2___sliceP2_faceon_lview_30Rsun_P1dir_bottom_0.1_10_RdBu_Run143.gif Faceon Mach number (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 30 31 … … 33 34 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run151/Mach_corot_rel_2___sliceP2_faceon_lview_30Rsun_P1dir_bottom_0.1_10_RdBu_Run151.gif Faceon Mach number (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 34 35 35 '''Figure 5fourth rowfaceon 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 nonrotating). Vectors show velocity field projected in orbital plane in coorbiting and corotating rest frame of particle 2:'''\\36 '''Figure 6 fourth rowfaceon 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 nonrotating). Vectors show velocity field projected in orbital plane in coorbiting and corotating rest frame of particle 2:'''\\ 36 37 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_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 Faceon normalized tangential velocity (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 37 38 … … 40 41 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_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 Faceon normalized tangential velocity (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\ 41 42 42 '''Figure 5fifth rowfaceon 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 coorbiting and corotating rest frame of particle 2:'''\\43 '''Figure 6 fifth rowfaceon 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 coorbiting and corotating rest frame of particle 2:'''\\ 43 44 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Postsink_particle/Postmodified_Lane_Emden/Run143/c_s_norm_vVec_corot_rel_2__sliceP2_faceon_lview_30Rsun_P1dir_bottom_0_8_caleblack_Run143.gif Faceon normalized sound speed (Model A: No subgrid accretion, M2 = 1 Msun)]\\ 44 45