Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24332
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Villaescusa-Navarro, Francisco | en_US |
dc.contributor.author | Planelles, Susana | en_US |
dc.contributor.author | BORGANI, STEFANO | en_US |
dc.contributor.author | VIEL, MATTEO | en_US |
dc.contributor.author | RASIA, ELENA | en_US |
dc.contributor.author | MURANTE, Giuseppe | en_US |
dc.contributor.author | Dolag, Klaus | en_US |
dc.contributor.author | Steinborn, Lisa K. | en_US |
dc.contributor.author | BIFFI, VERONICA | en_US |
dc.contributor.author | Beck, Alexander M. | en_US |
dc.contributor.author | Ragone-Figueroa, Cinthia | en_US |
dc.date.accessioned | 2020-04-29T14:31:45Z | - |
dc.date.available | 2020-04-29T14:31:45Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24332 | - |
dc.description.abstract | By means of zoom-in hydrodynamic simulations, we quantify the amount of neutral hydrogen (H I) hosted by groups and clusters of galaxies. Our simulations, which are based on an improved formulation of smoothed particle hydrodynamics, include radiative cooling, star formation, metal enrichment and supernova feedback, and can be split into two different groups, depending on whether feedback from active galactic nuclei (AGN) is turned on or off. Simulations are analysed to account for H I self-shielding and the presence of molecular hydrogen. We find that the mass in neutral hydrogen of dark matter haloes monotonically increases with the halo mass and can be well described by a power law of the form M_{H I}(M,z)∝ M^{3/4}. Our results point out that AGN feedback reduces both the total halo mass and its H I mass, although it is more efficient in removing H I. We conclude that AGN feedback reduces the neutral hydrogen mass of a given halo by ∼50 per cent, with a weak dependence on halo mass and redshift. The spatial distribution of neutral hydrogen within haloes is also affected by AGN feedback, whose effect is to decrease the fraction of H I that resides in the halo inner regions. By extrapolating our results to haloes not resolved in our simulations, we derive astrophysical implications from the measurements of Ω _{H I}(z): haloes with circular velocities larger than ∼25 km s<SUP>-1</SUP> are needed to host H I in order to reproduce observations. We find that only the model with AGN feedback is capable of reproducing the value of Ω _{H I}b_{H I} derived from available 21 cm intensity mapping observations. | en_US |
dc.language.iso | eng | en_US |
dc.title | Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stv2904 | en_US |
dc.identifier.scopus | 2-s2.0-84961737326 | en_US |
dc.identifier.isi | 000372265800011 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/456/4/3553/1032444 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 456 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 3553 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.456.3553V | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0001-6151-6439 | - |
crisitem.author.orcid | 0000-0002-2642-5707 | - |
crisitem.author.orcid | 0000-0003-4175-002X | - |
crisitem.author.orcid | 0000-0002-5155-130X | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
stv2904.pdf | pdf editoriale | 2.38 MB | Adobe PDF | View/Open |
Page view(s)
64
checked on Aug 31, 2024
Download(s)
22
checked on Aug 31, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.