Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26332
DC Field | Value | Language |
---|---|---|
dc.contributor.author | GREGGIO, Laura | en_US |
dc.contributor.author | FALOMO, Renato | en_US |
dc.contributor.author | USLENGHI, MICHELA | en_US |
dc.date.accessioned | 2020-07-03T14:05:46Z | - |
dc.date.available | 2020-07-03T14:05:46Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 9781107138193 | en_US |
dc.identifier.issn | 1743-9213 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26332 | - |
dc.description.abstract | Stellar halos around galaxies retain fundamental evidence of the processes which lead to their build up. Sophisticated models of galaxy formation in a cosmological context yield quantitative predictions about various observable characteristics, including the amount of substructure, the slope of radial mass profiles and three dimensional shapes, and the properties of the stellar populations in the halos. The comparison of such models with the observations provides constraints on the general picture of galaxy formation in the hierarchical Universe, as well as on the physical processes taking place in the halos formation. With the current observing facilities, stellar halos can be effectively probed only for a limited number of nearby galaxies. In this paper we illustrate the progress that we expect in this field with the future ground based large aperture telescopes (E-ELT) and with space based facilities as JWST. | en_US |
dc.language.iso | eng | en_US |
dc.title | Studying stellar halos with future facilities | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1017/S1743921315007024 | en_US |
dc.identifier.scopus | 2-s2.0-85030851198 | en_US |
dc.identifier.isi | 000450815700034 | en_US |
dc.identifier.url | https://doi.org/10.1017/S1743921315007024 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | vol. 11, S317 | en_US |
dc.relation.firstpage | 209 | en_US |
dc.relation.lastpage | 214 | en_US |
dc.relation.numberofpages | 6 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.numberofauthors | 3 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.alleditors | Bragaglia, Angela; Arnaboldi, Magda; Rejkuba, Marina; Romano, Donatella | en_US |
dc.relation.ispartofbook | The General Assembly of Galaxy Halos: Structure, Origin and Evolution | en_US |
dc.relation.conferencename | The General Assembly of Galaxy Halos: Structure, Origin and Evolution | en_US |
dc.relation.conferenceplace | Honolulu, Hawaii, USA | en_US |
dc.relation.conferencedate | 3-7 August, 2015 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | en_US |
dc.identifier.adsbibcode | 2016IAUS..317..209G | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0003-2634-4875 | - |
crisitem.author.orcid | 0000-0002-7585-8605 | - |
crisitem.journal.journalissn | 1743-9213 | - |
crisitem.journal.ance | E192651 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
iaus317_greggio_publ.pdf | 462.2 kB | Adobe PDF | View/Open | |
iaus317_greggio.pdf | 112.34 kB | Adobe PDF | View/Open |
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