We present a study of metal-enriched halo gas traced by Mg II and C IV absorption at z 1. It is clear from our results that environmental processes have a significant impact on the distribution of metals around galaxies and need to be fully accounted for when analysing correlations between gaseous haloes and galaxy properties
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
© 2022 ESO. This is the accepted manuscript version of an article which has been published in final ...
We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg II and C IV absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg II and C IV absorption at z 1. It is cle...
We present a study of the metal-enriched cool halo gas traced by Mg II absorption around 228 galaxie...
We present a study of the metal-enriched cool halo gas traced by Mg II absorption around 228 galaxie...
A growing population of metal absorbers are observed at z>5, many showing strong evolution in incide...
International audienceWe present a study of the metal-enriched halo gas, traced using MgII and [OII]...
Gas accreting onto a galaxy will be of low metallicity while halo gas due to a galactic fountain wil...
We present the first paper of the series Origin of Metals around Galaxies, which aims to explore the...
We present a detailed study of H I and metals for 110 Mg II absorption systems discovered at 1.98 12...
© 2022 ESO. This is the accepted manuscript version of an article which has been published in final ...
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
© 2022 ESO. This is the accepted manuscript version of an article which has been published in final ...
We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg II and C IV absorption at z 1. It is cle...
We present a study of metal-enriched halo gas traced by Mg II and C IV absorption at z 1. It is cle...
We present a study of the metal-enriched cool halo gas traced by Mg II absorption around 228 galaxie...
We present a study of the metal-enriched cool halo gas traced by Mg II absorption around 228 galaxie...
A growing population of metal absorbers are observed at z>5, many showing strong evolution in incide...
International audienceWe present a study of the metal-enriched halo gas, traced using MgII and [OII]...
Gas accreting onto a galaxy will be of low metallicity while halo gas due to a galactic fountain wil...
We present the first paper of the series Origin of Metals around Galaxies, which aims to explore the...
We present a detailed study of H I and metals for 110 Mg II absorption systems discovered at 1.98 12...
© 2022 ESO. This is the accepted manuscript version of an article which has been published in final ...
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
We present tomography of the circum-galactic metal distribution at redshift 1.7-4.5 derived from ech...
© 2022 ESO. This is the accepted manuscript version of an article which has been published in final ...