Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/25043
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Tacchella, S. | en_US |
dc.contributor.author | Carollo, C. M. | en_US |
dc.contributor.author | Renzini, A. | en_US |
dc.contributor.author | Schreiber, N. M. Förster | en_US |
dc.contributor.author | Lang, P. | en_US |
dc.contributor.author | Wuyts, S. | en_US |
dc.contributor.author | CRESCI, GIOVANNI | en_US |
dc.contributor.author | Dekel, A. | en_US |
dc.contributor.author | Genzel, R. | en_US |
dc.contributor.author | Lilly, S. J. | en_US |
dc.contributor.author | Mancini, C. | en_US |
dc.contributor.author | Newman, S. | en_US |
dc.contributor.author | Onodera, M. | en_US |
dc.contributor.author | Shapley, A. | en_US |
dc.contributor.author | Tacconi, L. | en_US |
dc.contributor.author | Woo, J. | en_US |
dc.contributor.author | Zamorani, G. | en_US |
dc.date.accessioned | 2020-05-21T11:29:25Z | - |
dc.date.available | 2020-05-21T11:29:25Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0036-8075 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/25043 | - |
dc.description.abstract | Most present-day galaxies with stellar masses ≥10<SUP>11</SUP> solar masses show no ongoing star formation and are dense spheroids. Ten billion years ago, similarly massive galaxies were typically forming stars at rates of hundreds solar masses per year. It is debated how star formation ceased, on which time scales, and how this “quenching” relates to the emergence of dense spheroids. We measured stellar mass and star-formation rate surface density distributions in star-forming galaxies at redshift 2.2 with ~1-kiloparsec resolution. We find that, in the most massive galaxies, star formation is quenched from the inside out, on time scales less than 1 billion years in the inner regions, up to a few billion years in the outer disks. These galaxies sustain high star-formation activity at large radii, while hosting fully grown and already quenched bulges in their cores. | en_US |
dc.language.iso | eng | en_US |
dc.title | Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1126/science.1261094 | en_US |
dc.identifier.scopus | 2-s2.0-84927720831 | en_US |
dc.identifier.isi | 000352999000038 | en_US |
dc.identifier.url | https://science.sciencemag.org/content/348/6232/314 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 348 | en_US |
dc.relation.issue | 6232 | en_US |
dc.relation.firstpage | 314 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015Sci...348..314T | 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.orcid | 0000-0002-5281-1417 | - |
crisitem.journal.journalissn | 0036-8075 | - |
crisitem.journal.ance | E151981 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
1504.04021.pdf | postprint | 6.56 MB | Adobe PDF | Visualizza/apri |
314.full.pdf | [Administrators only] | 1.4 MB | Adobe PDF |
Page view(s)
41
controllato il 1-mag-2024
Download(s)
13
controllato il 1-mag-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.