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Astronomy · L4 · Stellar structure: hydrostatic equilibrium and mass continuity · flowchart

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by @openstemUpdated Astronomy
Hydrostatic equilibriumdP/dr = −Gm(r)ρ(r)/r²Coupled system ofstellar structure equationsMass continuitydm/dr = 4πr²ρ(r)Equation of stateP = (ρ/μm_H)k_BTEnergy generationdL/dr = 4πr²ρεEnergy transport(radiative or convective)Full stellar structure model:P(r), ρ(r), T(r), m(r), L(r)

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