wiki:u/lchamandy

Version 5 (modified by Luke, 6 years ago) ( diff )

Movies Made Using Common Envelope Simulation Data

Paper I Paper II Paper 3: Chamandy+2019b (available soon)

Density (zoomed in) in lab frame

Face-on density (Model A: No subgrid accretion, M2 = 1 Msun)
Face-on density (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)
Face-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Movies corresponding to figures in Paper 1

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.

Figure 1/Figure 2—-face-on density:
Face-on density (Model A: No subgrid accretion, M2 = 1 Msun)

Face-on density (Model IB: Subgrid accretion, M2 = 1 Msun)

Face-on density (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Face-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Figure 4 top panel—-edge-on density:
Edge-on density (Model A: No subgrid accretion, M2 = 1 Msun)

Edge-on density (Model IB: Subgrid accretion, M2 = 1 Msun)

Edge-on density (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Edge-on density (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Figure 4 bottom panel—-edge-on density, zoomed in:
Edge-on density (zoomed in) (Model A: No subgrid accretion, M2 = 1 Msun)

Edge-on density (zoomed in) (Model IB: Subgrid accretion, M2 = 1 Msun)

Edge-on density (zoomed in) (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Edge-on density (zoomed in) (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Figure 6—-flow around companion:
Tangential velocity with velocity vectors (Model A: No subgrid accretion, M2 = 1 Msun)

Tangential velocity with velocity vectors (Model IB: Subgrid accretion, M2 = 1 Msun)

Tangential velocity with velocity vectors (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Tangential velocity with velocity vectors (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Movies corresponding to figures in paper 2

Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame.

Figure 3 top row—-face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors are velocity):
Face-on normalized energy (Model A: No subgrid accretion, M2 = 1 Msun)

Face-on normalized energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Face-on normalized energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

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 are velocity):
Face-on normalized kinetic energy (Model A: No subgrid accretion, M2 = 1 Msun)

Face-on normalized kinetic energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Face-on normalized kinetic energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Extra Movies

Temperature (Model A: No subgrid accretion, M2 = 1 Msun)

Temperature (Model IB: Subgrid accretion, M2 = 1 Msun)

Temperature (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)

Temperature (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)

Sound speed (Model A: No subgrid accretion, M2 = 1 Msun)

Sound speed (Model IB: Subgrid accretion, M2 = 1 Msun)

Mach, lab frame (Model A: No subgrid accretion, M2 = 1 Msun)

Mach, lab frame (Model IB: Subgrid accretion, M2 = 1 Msun)

Mach, frame corotating about secondary (Model A: No subgrid accretion, M2 = 1 Msun)

Mach, frame corotating about secondary (Model IB: Subgrid accretion, M2 = 1 Msun)

Side-by-side comparison of Model A (left) and Model IB (right) from Paper 1

Face-on density
Edge-on density
Edge-on density, zoomed
Tangential velocity
Temperature
Sound speed
Mach in lab frame
Mach in frame corotating about secondary

Note: See TracWiki for help on using the wiki.