Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analyti...
Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model
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Author / Creator
Zakharova, D , Vulcani, B , De Lucia, G , Finn, R A , Rudnick, G , Combes, F , Castignani, G , Fontanot, F , Jablonka, P , Xie, L and Hirschmann, M
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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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 environments. In this work, we examine the gas (atomic \ce{HI} and molecular \ce{H2}) content of local galax...
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Full title
Virgo Filaments. III. The gas content of galaxies in filaments as predicted by the GAEA semi-analytic model
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TN_cdi_proquest_journals_3099943390
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3099943390
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E-ISSN
2331-8422
