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Yields of Massive Stars and their Role in Galactic Chemical Evolution Studies
Nikos Prantzos
We review the yields of intermediate mass elements (from C to Zn) from massive stars and their associated uncertainties, in the light of recent theoretical results. We consider the…
Chemo-spectrophotometric evolution of spiral galaxies: III. Abundance and colour gradients in discs
N. Prantzos, S. Boissier
We study the relations between luminosity and chemical abundance profiles of spiral galaxies, using detailed models for the chemical and spectro-photometric evolution of galactic d…
Chemo-spectrophotometric evolution of spiral galaxies: II. Main properties of present day disk galaxies
S. Boissier, N. Prantzos
We study the chemical and spectro-photometric evolution of galactic disks with detailed models calibrated on the Milky Way and using simple scaling relations, based on currently po…
Cosmic radioactivities
Marcel Arnould, Nikos Prantzos
Radionuclides with half-lives ranging from some years to billions of years presumably synthesized outside of the solar system are now recorded in ``live'' or ``fossil'' form in var…
Chemo-spectrophotometric evolution of spiral galaxies: I. The model and the Milky Way
S. Boissier, N. Prantzos
The chemical and spectro-photometric evolution of spiral galaxies is investigated with detailed models, making use of up-to-date ingredients (like metallicity dependent stellar pro…
Gamma-Ray Line Astrophysics and Stellar Nucleosynthesis: Perspectives for INTEGRAL
N. Prantzos
Nuclear gamma-ray lines constitute the most genuine diagnostic tool of nuclear astrophysics, since they allow for an unambiguous identification of isotopic species. Continuous impr…