Fig. 1 from Ledoux Convection in Protoneutron Stars—A Clue to Supernova Nucleosynthesis?

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Ledoux Convection in Protoneutron Stars—A Clue to Supernova Nucleosynthesis?

Authors: Wolfgang Keil, H.-Thomas Janka, and Ewald Müller

Keil, Janka, & Müller 1996 The Astrophysical Journal Letters 473 L111.

Provider: AAS Journals

Caption: Fig. 1.

Convective (baryon) mass region inside the PNS vs. time for the two‐dimensional simulation. Black indicates regions that are Ledoux unstable or only marginally stable; gray denotes over‐ and undershooting regions where |v_θ| > 10⁷ cm s⁻¹.

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