International audienceWe show that simple models of the chemical and spectrophotometric evolution of galaxies can be used to explore the properties of present-day galaxies and especially the causes of the observed variety among disc galaxies. We focus on the link between `classical' spirals and Low Surface Brightness galaxies
Our statistical understanding of galaxy evolution is fundamentally driven by objects that lie above ...
We present mass models of a sample of 19 low surface brightness (LSB) galaxies and compare the prope...
Context. The distribution of chemical abundances and their variation with time are important tools ...
International audienceWe show that simple models of the chemical and spectrophotometric evolution of...
International audienceBased on the results of recent surveys, we have constructed a relatively homog...
Based on the results of recent surveys, we have constructed a relatively homogeneous set of observat...
A description is given of the samples of Low Surface Brightness galaxies (LSBs) used for comparison ...
We investigate the star formation history and chemical evolution of Low Surface Brightness (LSB) spi...
We investigate the star formation history and chemical evolution of low surface brightness (LSB) dis...
International audienceA description is given of the samples of Low Surface Brightness galaxies (LSBs...
Low Surface Brightness (LSB) galaxies are an important but often neglected part of the galaxy conten...
Abstract: Low Surface Brightness (LSB) galaxies form a large population of disc galaxies that extend...
International audienceWe present a study of the H I and optical properties of nearby (z ≤ 0.1) Low S...
14 pages, 11 figuresWe explore the implications for the high redshift universe of ``state-of-the-art...
11 pages, 8 figuresWe study the star formation history of normal spirals by using a large and homoge...
Our statistical understanding of galaxy evolution is fundamentally driven by objects that lie above ...
We present mass models of a sample of 19 low surface brightness (LSB) galaxies and compare the prope...
Context. The distribution of chemical abundances and their variation with time are important tools ...
International audienceWe show that simple models of the chemical and spectrophotometric evolution of...
International audienceBased on the results of recent surveys, we have constructed a relatively homog...
Based on the results of recent surveys, we have constructed a relatively homogeneous set of observat...
A description is given of the samples of Low Surface Brightness galaxies (LSBs) used for comparison ...
We investigate the star formation history and chemical evolution of Low Surface Brightness (LSB) spi...
We investigate the star formation history and chemical evolution of low surface brightness (LSB) dis...
International audienceA description is given of the samples of Low Surface Brightness galaxies (LSBs...
Low Surface Brightness (LSB) galaxies are an important but often neglected part of the galaxy conten...
Abstract: Low Surface Brightness (LSB) galaxies form a large population of disc galaxies that extend...
International audienceWe present a study of the H I and optical properties of nearby (z ≤ 0.1) Low S...
14 pages, 11 figuresWe explore the implications for the high redshift universe of ``state-of-the-art...
11 pages, 8 figuresWe study the star formation history of normal spirals by using a large and homoge...
Our statistical understanding of galaxy evolution is fundamentally driven by objects that lie above ...
We present mass models of a sample of 19 low surface brightness (LSB) galaxies and compare the prope...
Context. The distribution of chemical abundances and their variation with time are important tools ...
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