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Core-Collapse Supernovae and Compact Remnants

Stellar Structure and Evolution → Supernova Remnants and Observations

This advanced undergraduate astrophysics path covers the explosive death of massive stars, from core collapse and neutronization to supernova explosion mechanisms, neutrino emission, nucleosynthesis, and the resulting neutron stars, pulsars, and magnetars. It integrates stellar evolution, nuclear physics, and hydrodynamics to build a comprehensive understanding.

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14 steps · 14 nodes · 3 stages

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14 nodes26 edges3 relationships

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Path Steps

14 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

5 steps

Stage 2

Core Concepts

5 steps

Stage 3

Advanced Topics

4 steps

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