We studied the chemical properties of Milky-Way mass galaxies. We found common global chemical patterns with particularities which reflect their different assembly histories in a hierarchical scenario. We carried out a comprehensively analysis of the dynamical components (central spheroid, disc, inner and outer haloes) and their chemical properties
The primary present-day observables upon which theories of galaxy evolution are based are a system’s...
The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively str...
A model of chemical evolution for spheroidal systems is constructed assuming a relation between bind...
The chemical properties and abundance ratios of galaxies provide important information about their f...
One of the most important unsolved mysteries of astronomy is the formation and evolution of galaxies...
This thesis explores the chemical signatures of galaxy formation and evolution using a software pack...
A brief review of models of chemical evolution of the interstellar medium in our galaxy and other ga...
International audienceWe investigate the consequences of the hypothesis of the secular evolution (gr...
We show the results of a study using the spectral synthesis technique study to measure the chemical ...
We study the chemical properties of the stellar populations in eight simulations of the formation of...
Since stellar populations enhance particular element abundances according to the yields and lifetime...
Following a review of the basic ingredients necessary for constructing models of galactic chemical ...
A three-zone model of chemical evolution of our Galaxy is proposed to explain overall distribution o...
A short overview is presented of several topics concerning the evolution of the Milky Way (MW) in a ...
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in...
The primary present-day observables upon which theories of galaxy evolution are based are a system’s...
The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively str...
A model of chemical evolution for spheroidal systems is constructed assuming a relation between bind...
The chemical properties and abundance ratios of galaxies provide important information about their f...
One of the most important unsolved mysteries of astronomy is the formation and evolution of galaxies...
This thesis explores the chemical signatures of galaxy formation and evolution using a software pack...
A brief review of models of chemical evolution of the interstellar medium in our galaxy and other ga...
International audienceWe investigate the consequences of the hypothesis of the secular evolution (gr...
We show the results of a study using the spectral synthesis technique study to measure the chemical ...
We study the chemical properties of the stellar populations in eight simulations of the formation of...
Since stellar populations enhance particular element abundances according to the yields and lifetime...
Following a review of the basic ingredients necessary for constructing models of galactic chemical ...
A three-zone model of chemical evolution of our Galaxy is proposed to explain overall distribution o...
A short overview is presented of several topics concerning the evolution of the Milky Way (MW) in a ...
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in...
The primary present-day observables upon which theories of galaxy evolution are based are a system’s...
The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively str...
A model of chemical evolution for spheroidal systems is constructed assuming a relation between bind...
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