Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31502
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Cui, Weiguang | en_US |
dc.contributor.author | Knebe, Alexander | en_US |
dc.contributor.author | Yepes, Gustavo | en_US |
dc.contributor.author | Yang, Xiaohu | en_US |
dc.contributor.author | BORGANI, STEFANO | en_US |
dc.contributor.author | Kang, Xi | en_US |
dc.contributor.author | Power, Chris | en_US |
dc.contributor.author | Staveley-Smith, Lister | en_US |
dc.date.accessioned | 2022-02-28T15:31:14Z | - |
dc.date.available | 2022-02-28T15:31:14Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31502 | - |
dc.description.abstract | Using a series of cosmological simulations that includes one dark-matter-only (DM-only) run, one gas cooling-star formation-supernova feedback (CSF) run and one that additionally includes feedback from active galactic nuclei (AGNs), we classify the large-scale structures with both a velocity-shear-tensor code (VWEB) and a tidal-tensor code (PWEB). We find that the baryonic processes have almost no impact on large-scale structures - at least not when classified using aforementioned techniques. More importantly, our results confirm that the gas component alone can be used to infer the filamentary structure of the universe practically un-biased, which could be applied to cosmology constraints. In addition, the gas filaments are classified with its velocity (VWEB) and density (PWEB) fields, which can theoretically connect to the radio observations, such as H I surveys. This will help us to bias-freely link the radio observations with dark matter distributions at large scale. | en_US |
dc.language.iso | eng | en_US |
dc.title | The large-scale environment from cosmological simulations - I. The baryonic cosmic web | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx2323 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/473/1/68/4157280?login=true | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 473 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 68 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | USA | 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 | 2018MNRAS.473...68C | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0001-6151-6439 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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Items in DSpace are published in Open Access, unless otherwise indicated.