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MODELING SNR CASSIOPEIA A FROM THE SUPERNOVA EXPLOSION TO ITS CURRENT AGE: THE ROLE OF POST-EXPLOSION ANISOTROPIES OF EJECTA

  • Authors: S. Orlando, M. Miceli, M. L. Pumo, and F. Bocchino

2016 The Astrophysical Journal 822 22.

  • Provider: AAS Journals

Caption: Figure 12.

2D maps of average emission-measure-weighted velocity along the line of sight, vlos, for shocked Si/S (upper panel) and Fe (lower panel) derived from run CAS-15MS-1ETA. The approximate velocity range is ±4000 km s−1 (see color bar on the right in units of 103 km s−1). These images correspond to effective Doppler maps derived from observations. The black contour represents the projection of the remnant outline on the plane of the sky.

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