Free Access
Issue
A&A
Volume 654, October 2021
Article Number A167
Number of page(s) 18
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/202141569
Published online 26 October 2021

Movies

Movie 1: Density distribution for the ejecta of the model M60-V0-1Foe. The opaque irregular isosurface corresponds to a value of density which is at 1% of the peak density with one quadrant cut in order to see the radial distribution. The semi-transparent surface marks the position of the forward shock; the initially toroidal semi-transparent structures in red and cyan colors represent the inner and outer shells in the CSM, respectively. The system is oriented as G26, corresponding to the rotation angles ix = 30°, iy = 30°, iz = 25° about the x, y, and z axes, respectively.

Movie 2: Same as in Movie 1 but for the colors giving the radial velocity in units of 1000 km s−1 on the isosurface.

Movie 3: Same as in Movie 1 but for model M60-V0-9Foe.

Movie 4: Same as in Movie 3 but for the colors giving the radial velocity in units of 1000 km s−1 on the isosurface.


© ESO 2021

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