Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24663
DC Field | Value | Language |
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dc.contributor.author | HUNT, Leslie Kipp | en_US |
dc.contributor.author | Dayal, Pratika | en_US |
dc.contributor.author | MAGRINI, LAURA | en_US |
dc.contributor.author | Ferrara, Andrea | en_US |
dc.date.accessioned | 2020-05-08T15:21:35Z | - |
dc.date.available | 2020-05-08T15:21:35Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24663 | - |
dc.description.abstract | With the aim of understanding the coevolution of star formation rate (SFR), stellar mass (M<SUB>*</SUB>), and oxygen abundance (O/H) in galaxies up to redshift z ≃ 3.7, we have compiled the largest available data set for studying Metallicity Evolution and Galaxy Assembly (MEGA); it comprises ∼1000 galaxies with a common O/H calibration and spans almost two orders of magnitude in metallicity, a factor of ∼10<SUP>6</SUP> in SFR, and a factor of ∼10<SUP>5</SUP> in stellar mass. From a principal component analysis, we find that the three-dimensional parameter space reduces to a Fundamental Plane in metallicity (FPZ) given by 12 + log (O/H) = -0.14 log (SFR) + 0.37 log (M<SUB>*</SUB>) + 4.82. The mean O/H FPZ residuals are small (0.16 dex) and consistent with trends found in smaller galaxy samples with more limited ranges in M<SUB>*</SUB>, SFR, and O/H. Importantly, the FPZ is found to be approximately redshift invariant within the uncertainties. In a companion paper, these results are interpreted with an updated version of the model presented by Dayal, Ferrara & Dunlop. | en_US |
dc.language.iso | eng | en_US |
dc.title | Coevolution of metallicity and star formation in galaxies to z ≃ 3.7 - I. A Fundamental Plane | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw1993 | en_US |
dc.identifier.scopus | 2-s2.0-85029527120 | en_US |
dc.identifier.isi | 000388122400067 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/463/2/2002/2892244 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 463 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2002 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | 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.463.2002H | 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. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0001-9162-2371 | - |
crisitem.author.orcid | 0000-0003-4486-6802 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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2016MNRAS-2002-19Hunt.pdf | PDF editoriale | 3 MB | Adobe PDF | View/Open |
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