Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30297
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Oskari Miettinen | en_US |
dc.contributor.author | DELVECCHIO, IVAN | en_US |
dc.contributor.author | Vernesa Smolčić | en_US |
dc.contributor.author | Manuel Aravena | en_US |
dc.contributor.author | Drew Brisbin | en_US |
dc.contributor.author | Alexander Karim | en_US |
dc.date.accessioned | 2021-02-10T15:50:00Z | - |
dc.date.available | 2021-02-10T15:50:00Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30297 | - |
dc.description.abstract | The star formation rate per unit area correlates well with the gas surface density for different types of galaxies. However, this Kennicutt-Schmidt law has not yet been examined for a large, homogeneously selected sample of SMGs, which could provide useful SF implementation information for models of massive galaxy formation and evolution. We aim at determining the K-S law parameters for the first time for a well-selected, statistical sample of SMGs. We used ALMA to conduct a 0.2" resolution, 870 $\mu$m imaging survey of 40 SMGs in COSMOS, which were initially selected at 1.1 mm. We analysed a sample of 32/40 target SMGs, for which our new ALMA 870 $\mu$m data provide information about the spatial extent of dust emission, and all of which have dust-obscured SFR and dust-based gas mass estimates available from our previous study. We divided our sample into equally large subsamples of main-sequence objects and starbursts, and found their K-S relations to be of the form $\Sigma_{\rm SFR} \propto \Sigma_{\rm gas}^{0.81\pm0.01}$ and $\Sigma_{\rm SFR} \propto \Sigma_{\rm gas}^{0.84\pm0.39}$, respectively. The slightly sub-linear K-S slopes we derived suggest that the SF efficiency is nearly constant across the $\Sigma_{\rm gas}$ range probed. Under the assumption of a Galactic CO-to-H$_2$ conversion factor for the whole sample, the MS SMGs obey a constant global SFE of about 21% per 100 Myr, while that of starburst SMGs is about 27%. The corresponding gas depletion times are $\sim480$ Myr and 370 Myr. On average, our SMGs have $\Sigma_{\rm gas}\gtrsim10^{3.9}$ M$_{\odot}$ pc$^{-2}$, which suggests that they are Eddington-limited. This is consistent with the theoretical expectation of a linear K-S relation for such systems. However, size measurements of the CO-emitting regions of SMGs, and the $\alpha_{\rm CO}$ values of SMGs are needed to further constrain their $\Sigma_{\rm gas}$ values. | en_US |
dc.language.iso | eng | en_US |
dc.title | On the Kennicutt-Schmidt scaling law of submillimetre galaxies | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201731157 | en_US |
dc.identifier.scopus | 2-s2.0-85020877499 | en_US |
dc.identifier.isi | 000404648300140 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/full_html/2017/06/aa31157-17/aa31157-17.html | en_US |
dc.identifier.url | http://arxiv.org/abs/1706.00589v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 602 | en_US |
dc.relation.firstpage | L9 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.description.apc | sì | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0001-8706-2252 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Miettinen_KS2017.pdf | pdf editoriale | 1.03 MB | Adobe PDF | View/Open |
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