Emanuele Spitoni
pure.au.dk
0000-0001-9715-5727
Aarhus University
41 papers found
Refreshing results…
A simple and general method for solving detailed chemical evolution with delayed production of iron and other chemical elements
Are ancient dwarf satellites the building blocks of the Galactic halo?
The effect of radial gas flows on the chemical evolution of galaxies (The Milky Way and M31)
New chemical evolution analytical solutions including environment effects
The Effect of Stellar Migration on Galactic Chemical Evolution: A Heuristic Approach
Chemical evolution of the bulge of M31: predictions about abundance ratios
Chemical Evolution of M31
The galactic habitable zone of the Milky Way and M31 from chemical evolution models with gas radial flows
The effect of radial gas flows on the chemical evolution of the Milky Way and M31
Abundance gradients in spiral discs: is the gradient inversion at high redshift real?
Galactic and cosmic Type Ia supernova (SNIa) rates: is it possible to impose constraints on SNIa progenitors?
Effects of the radial inflow of gas and galactic fountains on the chemical evolution of M 31
The thick disk rotation-metallicity correlation as a fossil of an “inverse chemical gradient” in the early Galaxy
ISM simulations: an overview of models
Electron distribution in the Galactic disc: results from a non-equilibrium ionization model of the interstellar medium
Effects of the radial flows on the chemical evolution of the Milky Way disk
The origin of the mass-metallicity relation: an analytical approach
Effects of galactic fountains and delayed mixing in the chemical evolution of the Milky Way
The effect of different type Ia supernova progenitors on Galactic chemical evolution
The effect of differential galactic winds on the chemical evolution of galaxies
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