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Introduction Method Data Analysis and Results Conclusions

We present in this contribution the predictions on the multiwavelength spectral energy distribution of our evolutionary population synthesis models including single and binary stellar systems. The high energy computations include the emission associated to X-ray binaries and supernovae remnants, as well as the mechanical energy released into the

This article presents a theoretical framework for the evolution of light element nuclides in the Galactic disc. The authors use two key assumptions: infall of metal-poor gas to the disc at an increasing rate, and destruction of fragile nuclides in hot relatively dense supergiant envelopes. Light nuclides are accelerated by supernova shocks, and

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