Outputs (3)

Ram pressure stripping in the z  ∼  0.5 galaxy cluster MS 0451.6-0305 (2022)
Journal Article
Durret, F., Degott, L., Lobo, C., Ebeling, H., Jauzac, M., & Tam, S.-I. (2022). Ram pressure stripping in the z  ∼  0.5 galaxy cluster MS 0451.6-0305. Astronomy & Astrophysics, 662, Article A84. https://doi.org/10.1051/0004-6361/202142983

The pressure exerted by the ambient hot X-ray gas on cluster galaxies can lead to the presence of ram pressure stripped (RPS) galaxies, characterized by asymmetric shapes, and, in some cases, tails of blue stars and/or X-ray gas, with increased star... Read More about Ram pressure stripping in the z  ∼  0.5 galaxy cluster MS 0451.6-0305.

Pilot-WINGS: An extended MUSE view of the structure of Abell 370 (2022)
Journal Article
Lagattuta, D. J., Richard, J., Bauer, F. E., Cerny, C., Claeyssens, A., Guaita, L., Jauzac, M., Jeanneau, A., Koekemoer, A. M., Mahler, G., Prieto Lyon, G., Acebron, A., Meneghetti, M., Niemiec, A., Zitrin, A., Bianconi, M., Connor, T., Cen, R., Edge, A., Faisst, A. L., …Weaver, J. R. (2022). Pilot-WINGS: An extended MUSE view of the structure of Abell 370. Monthly Notices of the Royal Astronomical Society, 514(1), 497-517. https://doi.org/10.1093/mnras/stac418

We investigate the strong-lensing cluster Abell 370 (A370) using a wide Integral Field Unit (IFU) spectroscopic mosaic from the Multi-Unit Spectroscopic Explorer (MUSE). IFU spectroscopy provides significant insight into the structure and mass conten... Read More about Pilot-WINGS: An extended MUSE view of the structure of Abell 370.

Scatter in the satellite galaxy SHMR: fitting functions, scaling relations, and physical processes from the IllustrisTNG simulation (2022)
Journal Article
Niemiec, A., Giocoli, C., Cohen, E., Jauzac, M., Jullo, E., & Limousin, M. (2022). Scatter in the satellite galaxy SHMR: fitting functions, scaling relations, and physical processes from the IllustrisTNG simulation. Monthly Notices of the Royal Astronomical Society, 512(4), 6021-6037. https://doi.org/10.1093/mnras/stac832

The connection between galaxies and their dark matter haloes is often described with the stellar-to-halo mass relation (SHMR). Satellite galaxies in clusters follow an SHMR distinct from central galaxies because of the environmental processes that th... Read More about Scatter in the satellite galaxy SHMR: fitting functions, scaling relations, and physical processes from the IllustrisTNG simulation.