F. Combes

most citedSEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1

-

1148 at

z \sim 0.5

10 citations · 10 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.GA2024

Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model

D. Zakharova, B. Vulcani, G. De Lucia +8

Galaxy evolution depends on the environment in which galaxies are located. The various physical processes (ram-pressure stripping, tidal interactions, etc.) that can affect the gas…

astro-ph.GA2021★ 10 cited

SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1 $-$ 1148 at $z \sim 0.5$

D. Spérone-Longin, P. Jablonka, F. Combes +7

We investigate how the galaxy reservoirs of molecular gas fuelling star formation are transformed while the host galaxies infall onto galaxy cluster cores. As part of the Spatially…

Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model

SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1−1148 at z∼0.5

SEEDisCS I. Molecular gas in galaxy clusters and their large scale structure: the case of CL1411.1 $-$ 1148 at $z \sim 0.5$