Changes between Version 14 and Version 15 of u/lchamandy


Ignore:
Timestamp:
11/26/19 12:08:01 (5 years ago)
Author:
Luke
Comment:

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  • u/lchamandy

    v14 v15  
    33[https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.1898C/abstract Paper I: Chamandy+2018 "Accretion in Common Envelope Evolution"]\\
    44[https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1070C/abstract Paper II: Chamandy+2019a "Energy Budget and Core-Envelope Motion in Common Envelope Evolution"]\\
    5 [https://arxiv.org/abs/1908.06195 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"]
    66
    77== Density (zoomed in) in lab frame ==
    … …  
    1212== 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.
    1313
    14 '''Figure 5 first row---face-on force density in units of 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):'''\\
     14'''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):'''\\
    1515[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)]\\
    1616