Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29494
DC Field | Value | Language |
---|---|---|
dc.contributor.author | VALIANTE, ROSA | en_US |
dc.contributor.author | Gioannini, L. | en_US |
dc.contributor.author | Schneider, R. | en_US |
dc.contributor.author | Matteucci, F. | en_US |
dc.contributor.author | Dell'Agli, Flavia | en_US |
dc.contributor.author | DI CRISCIENZO, Marcella | en_US |
dc.date.accessioned | 2021-01-05T15:12:59Z | - |
dc.date.available | 2021-01-05T15:12:59Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0037-8720 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29494 | - |
dc.description.abstract | Far infrared and sub-millimeter observations of quasars and normal star forming galaxies at z>6 have revealed the presence of large amounts of dust. At such high redshifts, the inferred 10<SUP>7</SUP>-10<SUP>9</SUP> M_☉ masses of dust must have formed in less than one billion years. Explaining this rapid chemical evolution is a challenge for both observations and theoretical models. Here we discuss the relative role of the two main stellar sources, AGB stars and SNe, in early dust enrichment, in light of new theoretical dust yields for AGB stars. | en_US |
dc.language.iso | eng | en_US |
dc.title | The relative role of AGB stars and SNe as the first cosmic dust polluters | en_US |
dc.type | Article | - |
dc.identifier.url | http://sait.oat.ts.astro.it/MSAIt880317/index.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 88 | en_US |
dc.relation.firstpage | 420 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MEMORIE DELLA SOCIETA ASTRONOMICA ITALIANA | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017MmSAI..88..420V | 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. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0003-3050-1765 | - |
crisitem.author.orcid | 0000-0003-2442-6981 | - |
crisitem.author.orcid | 0000-0003-4132-1209 | - |
crisitem.journal.journalissn | 0037-8720 | - |
crisitem.journal.ance | E108779 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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2017MmSAI__88__420V.pdf | Pdf editoriale | 336.31 kB | Adobe PDF | View/Open |
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