Zobrazeno 1 - 10
of 2 719
pro vyhledávání: '"Finn, R."'
Autor:
Zakharova, D., Vulcani, B., De Lucia, G., Finn, R. A., Rudnick, G., Combes, F., Castignani, G., Fontanot, F., Jablonka, P., Xie, L., Hirschmann, M.
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 content in galaxies have different efficiencies in different environm
Externí odkaz:
http://arxiv.org/abs/2408.17367
Autor:
Castignani, G., Vulcani, B., Finn, R. A., Combes, F., Jablonka, P., Rudnick, G., Zaritsky, D., Whalen, K., Conger, K., De Lucia, G., Desai, V., Koopmann, R. A., Moustakas, J., Norman, D. J., Townsend, M.
Virgo is the nearest galaxy cluster; it is thus ideal for studies of galaxy evolution in dense environments in the local Universe. It is embedded in a complex filamentary network of galaxies and groups, which represents the skeleton of the large scal
Externí odkaz:
http://arxiv.org/abs/2110.13797
Autor:
Spérone-Longin, D., Jablonka, P., Combes, F., Castignani, G., Krips, M., Rudnick, G., Desjardins, T., Zaritsky, D., Finn, R. A., De Lucia, G., Desai, V.
Publikováno v:
A&A 654, A69 (2021)
This paper is the second of a series that tackles the properties of molecular gas in galaxies residing in clusters and their related large-scale structures. Out of 21 targeted fields, 19 galaxies were detected in CO(3-2) with the Atacama Large Millim
Externí odkaz:
http://arxiv.org/abs/2105.02663
Autor:
Castignani, G., Combes, F., Jablonka, P., Finn, R. A., Rudnick, G., Vulcani, B., Desai, V., Zaritsky, D., Salomé, P.
Publikováno v:
A&A 657, A9 (2022)
Galaxies have different morphology, gas content and star formation rate (SFR) in dense environments like galaxy clusters. The impact of environmental density extends to several virial radii, and galaxies are pre-processed in filaments and groups, bef
Externí odkaz:
http://arxiv.org/abs/2101.04389