Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31794
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | DE LUCIA, GABRIELLA | en_US |
dc.date.accessioned | 2022-03-22T14:39:03Z | - |
dc.date.available | 2022-03-22T14:39:03Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 2075-4434 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31794 | - |
dc.description.abstract | Previous chapters of this issue have focused on the formation and evolution of cosmic structures under the influence of gravity alone. In order to make a close link between theoretical models of structure formation and observational data, it is necessary to consider the gas-dynamical and radiative processes that drive the evolution of the baryonic components of dark matter halos. These processes cover many orders of magnitude in physical sizes and time-scales and are entangled in a complex network of actions, back-reactions, and self-regulations. In addition, our understanding of them is far from being complete, even when viewed in isolation. This chapter provides a brief review of the techniques that are commonly used to link the physical properties of galaxies with the dark matter halos in which they reside. I discuss the main features of these methods, as well as their aims, limits, and complementarities. | en_US |
dc.language.iso | eng | en_US |
dc.title | Lighting up dark matter haloes | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3390/GALAXIES7020056 | en_US |
dc.identifier.scopus | 2-s2.0-85069970536 | en_US |
dc.identifier.url | https://www.mdpi.com/2075-4434/7/2/56/htm | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85069970536 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 7 | en_US |
dc.relation.issue | 2 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | GALAXIES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0002-6220-9104 | - |
crisitem.journal.journalissn | 2075-4434 | - |
crisitem.journal.ance | E222261 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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galaxies-07-00056.pdf | Pdf editoriale | 3.31 MB | Adobe PDF | Visualizza/apri |
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