Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24663
DC Field | Value | Language |
---|---|---|
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.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. Arcetri | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0001-9162-2371 | - |
crisitem.author.orcid | 0000-0003-4486-6802 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2016MNRAS-2002-19Hunt.pdf | PDF editoriale | 3 MB | Adobe PDF | View/Open |
Page view(s)
60
checked on Jul 27, 2024
Download(s)
12
checked on Jul 27, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.