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 use the most extensive integral field spectroscopic map of a local galaxy, NGC 628, combined with...
We study the physical conditions of the circumgalactic medium (CGM) around z = 0.25 galaxies as trac...
International audienceWe now have mounting evidences that the circumgalactic medium (CGM) of galaxie...
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...
Gas accreting onto a galaxy will be of low metallicity while halo gas due to a galactic fountain wil...
International audienceWe present a study of the metal-enriched halo gas, traced using MgII and [OII]...
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...
The metallicity structure of galactic haloes is one of the major unknowns in modern galactic astr...
We examine the properties of two galaxy "halos" at z ~ 0.7 in the TON 153 (z_em = 1.01) quasar field...
Gas-phase metallicity derived from absorption profiles may hold a unique key into the origins of the...
With the installation of the Cosmic Origins Spectrograph on the Hubble Space Telescope, measurements...
We use the most extensive integral field spectroscopic map of a local galaxy, NGC 628, combined with...
We study the physical conditions of the circumgalactic medium (CGM) around z = 0.25 galaxies as trac...
International audienceWe now have mounting evidences that the circumgalactic medium (CGM) of galaxie...
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...
Gas accreting onto a galaxy will be of low metallicity while halo gas due to a galactic fountain wil...
International audienceWe present a study of the metal-enriched halo gas, traced using MgII and [OII]...
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...
The metallicity structure of galactic haloes is one of the major unknowns in modern galactic astr...
We examine the properties of two galaxy "halos" at z ~ 0.7 in the TON 153 (z_em = 1.01) quasar field...
Gas-phase metallicity derived from absorption profiles may hold a unique key into the origins of the...
With the installation of the Cosmic Origins Spectrograph on the Hubble Space Telescope, measurements...
We use the most extensive integral field spectroscopic map of a local galaxy, NGC 628, combined with...
We study the physical conditions of the circumgalactic medium (CGM) around z = 0.25 galaxies as trac...
International audienceWe now have mounting evidences that the circumgalactic medium (CGM) of galaxie...