Fig. 5 from An Investigation of Neutrino‐driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino Transport

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An Investigation of Neutrino‐driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino Transport

Authors: A Mezzacappa, A. C. Calder, S. W. Bruenn, J. M. Blondin, M. W. Guidry, M. R. Strayer, and A. S. Umar

Mezzacappa et al. 1998 The Astrophysical Journal 495 911.

Provider: AAS Journals

Caption: Fig. 5.

(a) Two‐dimensional radial velocity plots showing the evolution of ND convection in our 15 M_☉ model, at 137, 212, and 512 ms after bounce. (b) Plots of the angle‐averaged radial velocity for the three radial velocity snapshots shown in Fig. 4a. Also shown for comparison is the corresponding radial velocity from our one‐dimensional PPM simulation.

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