We present the results of a pilot XMM-Newton and Chandra program aimed at studying the diffuse intragroup medium (IGM) of optically selected nearby groups from the Zurich ENvironmental Study (ZENS) catalog. The groups are in a narrow mass range about 10(13) M-circle dot, a mass scale at which the interplay between the IGM and the group member galaxies is still largely unprobed. X-ray emission from the IGM is detected in the energy band 0.5-2 keV with fluxPeer reviewe
We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightli...
Galaxy groups and low-mass clusters provide important laboratories in which to study X-ray gas physi...
Context. Observations of the formation and evolution of massive galaxy clusters and their ...
In this thesis, we have explored what information may be gleaned from X-ray observations of galaxies...
Isolated compact groups (CGs) of galaxies present a range of dynamical states, group velocity disper...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
We have undertaken a multiwavelength project to study the relatively unknown properties of groups an...
The Hickson compact groups, displaying regions of high galaxy densities, should provide environments...
The Zurich Environmental Study (ZENS) is based on a sample of ~1500 galaxy members of 141 groups in ...
Galaxy groups are more than an intermediate scale between clusters and halos hosting individual gala...
The fraction of galaxies bound in groups in the nearby Universe is high (50% at z~0). Systematic stu...
We present an analysis of the diffuse X-ray emission in 19 compact groups (CGs) of galaxies observed...
We present the results of spectroscopic observations of galaxies associated with the diffuse X-ray e...
Galaxies in compact groups tend to be deficient in neutral hydrogen compared to isolated galaxies of...
We present the results of the 2-dimensional XMM-Newton Group Survey (2dXGS), an archival study of ne...
We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightli...
Galaxy groups and low-mass clusters provide important laboratories in which to study X-ray gas physi...
Context. Observations of the formation and evolution of massive galaxy clusters and their ...
In this thesis, we have explored what information may be gleaned from X-ray observations of galaxies...
Isolated compact groups (CGs) of galaxies present a range of dynamical states, group velocity disper...
Our understanding of how active galactic nucleus feedback operates in galaxy clusters has improved i...
We have undertaken a multiwavelength project to study the relatively unknown properties of groups an...
The Hickson compact groups, displaying regions of high galaxy densities, should provide environments...
The Zurich Environmental Study (ZENS) is based on a sample of ~1500 galaxy members of 141 groups in ...
Galaxy groups are more than an intermediate scale between clusters and halos hosting individual gala...
The fraction of galaxies bound in groups in the nearby Universe is high (50% at z~0). Systematic stu...
We present an analysis of the diffuse X-ray emission in 19 compact groups (CGs) of galaxies observed...
We present the results of spectroscopic observations of galaxies associated with the diffuse X-ray e...
Galaxies in compact groups tend to be deficient in neutral hydrogen compared to isolated galaxies of...
We present the results of the 2-dimensional XMM-Newton Group Survey (2dXGS), an archival study of ne...
We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightli...
Galaxy groups and low-mass clusters provide important laboratories in which to study X-ray gas physi...
Context. Observations of the formation and evolution of massive galaxy clusters and their ...