Formation of the Halo Stellar Population in Spiral and Elliptical Galaxies (original) (raw)

Lecture Notes in Physics, 2003

Abstract

... k=1 mbk [Qi(τj,k) − Qi(τj−1,k)] (6) ms(tbj ) = ms(tbj−1 ) + mbj−1 − j−1 ∑ k=1 mbk [Qm(τj,k) − Qm(τj−1,k)] (7) where τj,k = tbj − tbk τj−1,k = tbj−1 − tbk , ... In order to test the validity of thebuilding-up numerical model we carried out a comparison of numerical results with analytical. ...

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