A closed-form formula for star formation histories in galactocentric radial shells is derived from empirical galaxy scaling relations and two star formation history models.
(3) analytically for arbitrary S´ ersic indices is mathematically rather challenging, ρ⋆(r) = − 1 π Z ∞ r dΣ dR dR√ R2 − r2
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Dark-matter-induced transients over cosmic time: The role of star formation history profiles
A closed-form formula for star formation histories in galactocentric radial shells is derived from empirical galaxy scaling relations and two star formation history models.