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The Origin of the Stellar Mass Distribution and Multiplicity
(Springer, 2020)
Mass loss and expansion of ultra compact dwarf galaxies through gas expulsion and stellar evolution for top-heavy stellar initial mass functions
(WILEY-BLACKWELL PUBLISHING, INC, 2010)
The stellar metallicity gradients in galaxy discs in a cosmological scenario
(2016)
Context. The stellar metallicity gradients of disc galaxies provide information on disc assembly, star formation processes, and chemical evolution. They also might store information on dynamical processes that could affect ...
The Mass of the Most Massive Star in Stellar Clusters Determined from 25 Million MASSCLEAN Monte Carlo Simulations
(2013)
Is there a maximum universal stellar mass, or might the maximum stellar mass in a cluster be tied to the mass of the associated cluster? Direct measurements of the maximum stellar mass of hundreds of young stellar clusters ...
SELECTED TOPICS IN THE EVOLUTION OF LOW-MASS STARS
(S/EDITORIAL, 2013)
Low-mass stars play a key role in many different areas of astrophysics. In this
article, I provide a brief overview of the evolution of low-mass stars, and discuss some of
the uncertainties and problems currently affecting ...
The Gaia–ESO Survey: Carbon Abundance in the Galactic Thin and Thick Disks
(The American Astronomical Society, 2020)
This paper focuses on carbon, which is one of the most abundant elements in the universe and is of high importance in the field of nucleosynthesis and galactic and stellar evolution. The origin of carbon and the relative ...