Titlebook: Chemical Evolution of Galaxies; Francesca Matteucci Book 2012 Springer-Verlag Berlin Heidelberg 2012 Chemical Evolution of Galaxies.Classi

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A Historical Glimpse and Stalwartslar galaxies could also be important contributors to the population of systems giving rise to QSO-absorption lines at high redshift, in particular the damped-Lyman-α systems.In this chapter, we also show the mass–metallicity relation found for star forming galaxies at low and high redshift and discuss some possible interpretations.

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Simple Models of Chemical Evolution, need to be made. We show first the solution of the . and then more complex solutions for cases with galactic flows such as outflow, infall, and radial inflow. We also show the failure of analytical models in reproducing the observations.

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Chemical Evolution of Early Type Galaxies, stellar populations are derived. The evolution of ellipticals hosting quasars is discussed. The properties of dwarf spheroidal galaxies in the local group are discussed, and by comparing the predicted and observed abundances, we try to understand whether they could have been the building blocks of the Milky Way.

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Introduction, some .Li during spallation processes, which derive from the interaction between cosmic rays and interstellar atoms of carbon (C), nitrogen (N), and oxygen (O). All the elements with . ≥ 12 starting from .C have been synthesized inside the stars and the sum of all of them in Astronomy is called . and indicated with capital ..

Boycott

Chemical Evolution of the Milky Way and Other Spirals, more detail. Observational data on spiral galaxies suggest that there has been a downsizing in the star formation, in the sense that the most massive spirals should have formed more quickly and with a more efficient star formation than the less massive ones, and therefore they should be older.

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