Cosmic Star Formation from the Milky Way and its Satellites

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Minor revisions. 6 pages, 5 figures, Latex, uses paspconf.sty, Invited contribution to IAU Symposium 190-New Views of the Mage

Scientific paper

We use observations and evolutionary models of local objects to interpret a
recent determination of the star-formation history of the universe. By fitting
the global star-formation rate, the model predicts the ratio of spheroid to
disk mass of $\sim$1, an intergalactic medium (IGM) whose mass is $\sim$2.3
times the mass in stars, and whose metallicity is $\sim$0.1 Z$_\odot$.

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