International audienceContext. In a galaxy cluster, the evolution of spiral galaxies depends on their cluster environment. Ram pressure due to the rapid motion of a spiral galaxy within the hot intracluster medium removes the galaxy's interstellar medium from the outer disk. Once the gas has left the disk, star formation stops. The passive evolution of the stellar populations should be detectable in optical spectroscopy and multi-wavelength photometry. Aims. The goal of our study is to recover the stripping age of the Virgo spiral galaxy NGC 4388, i.e. the time elapsed since the halt of star formation in the outer galactic disk using a combined analysis of optical spectra and photometry. Methods. We performed VLT FORS2 long-slit spectroscop...
International audienceWe study the star formation quenching mechanism in cluster galaxies by fitting...
International audienceThe influence of the environment on gas surface density and star formation eff...
We present a new method for studying the star formation history of late-type cluster galaxies underg...
International audienceContext. In a galaxy cluster, the evolution of spiral galaxies depends on thei...
Context. In a galaxy cluster, the evolution of spiral galaxies depends on their cluster environment....
This thesis investigates the influence of ram pressure stripping on the star formation history of cl...
International audienceSince the Virgo cluster is the closest galaxy cluster in the northern hemisphe...
accepted by ApJ With multiband photometric data in public archives, we detected four intracluster st...
Accepted for publication on ApJWe present a new method for studying the star formation history of la...
International audienceGas can be violently stripped from their galaxy disks in rich clusters, and be...
Cette thèse étudie l'influence du balayage par pression dynamique sur l'histoire de la formation ste...
International audienceIt has been shown that the Virgo spiral galaxy NGC 4330 shows signs of ongoing...
International audienceNGC 4330 is one of the Virgo galaxies whose UV emission distributions show a t...
International audienceThe Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a bli...
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-band Hα + [N...
International audienceWe study the star formation quenching mechanism in cluster galaxies by fitting...
International audienceThe influence of the environment on gas surface density and star formation eff...
We present a new method for studying the star formation history of late-type cluster galaxies underg...
International audienceContext. In a galaxy cluster, the evolution of spiral galaxies depends on thei...
Context. In a galaxy cluster, the evolution of spiral galaxies depends on their cluster environment....
This thesis investigates the influence of ram pressure stripping on the star formation history of cl...
International audienceSince the Virgo cluster is the closest galaxy cluster in the northern hemisphe...
accepted by ApJ With multiband photometric data in public archives, we detected four intracluster st...
Accepted for publication on ApJWe present a new method for studying the star formation history of la...
International audienceGas can be violently stripped from their galaxy disks in rich clusters, and be...
Cette thèse étudie l'influence du balayage par pression dynamique sur l'histoire de la formation ste...
International audienceIt has been shown that the Virgo spiral galaxy NGC 4330 shows signs of ongoing...
International audienceNGC 4330 is one of the Virgo galaxies whose UV emission distributions show a t...
International audienceThe Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a bli...
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-band Hα + [N...
International audienceWe study the star formation quenching mechanism in cluster galaxies by fitting...
International audienceThe influence of the environment on gas surface density and star formation eff...
We present a new method for studying the star formation history of late-type cluster galaxies underg...