Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32281
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Q. D'Amato | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | BRIENZA, MARISA | en_US |
dc.contributor.author | GILLI, Roberto | en_US |
dc.contributor.author | C. Vignali | en_US |
dc.contributor.author | Paladino, Rosita | en_US |
dc.contributor.author | LOI, FRANCESCA | en_US |
dc.contributor.author | MASSARDI, MARCELLA | en_US |
dc.contributor.author | MIGNOLI, Marco | en_US |
dc.contributor.author | MARCHESI, STEFANO | en_US |
dc.contributor.author | PECA, ALESSANDRO | en_US |
dc.contributor.author | P. Jagannathan | en_US |
dc.date.accessioned | 2022-06-10T14:55:54Z | - |
dc.date.available | 2022-06-10T14:55:54Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 2075-4434 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32281 | - |
dc.description.abstract | In this work we performed a spectral energy distribution (SED) analysis in the optical/infrared band of the host galaxy of a proto-brightest cluster galaxy (BCG, NVSS J103023+052426) in a proto-cluster at z = 1.7. We found that it features a vigorous star formation rate (SFR) of ${\sim}$570 $\mathrm{M_{\odot}}$/yr and a stellar mass of $M_{\ast} \sim 3.7 \times 10^{11}$ $\mathrm{M_{\odot}}$; the high corresponding specific SFR = $1.5 \pm 0.5$ $\mathrm{Gyr^{-1}}$ classifies this object as a starburst galaxy that will deplete its molecular gas reservoir in $\sim$ $3.5 \times 10^8$ yr. Thus, this system represents a rare example of a proto-BCG caught during the short phase of its major stellar mass assembly. Moreover, we investigated the nature of the host galaxy emission at 3.3 mm. We found that it originates from the cold dust in the interstellar medium, even though a minor non-thermal AGN contribution cannot be completely ruled out. Finally, we studied the polarized emission of the lobes at 1.4 GHz. We unveiled a patchy structure where the polarization fraction increases in the regions in which the total intensity shows a bending morphology; in addition, the magnetic field orientation follows the direction of the bendings. We interpret these features as possible indications of an interaction with the intracluster medium. This strengthens the hypothesis of positive AGN feedback, as inferred in previous studies of this object on the basis of X-ray/mm/radio analysis. In this scenario, the proto-BCG heats the surrounding medium and possibly enhances the SFR in nearby galaxies. | en_US |
dc.language.iso | eng | en_US |
dc.title | Multi-Wavelength Study of a Proto-BCG at z = 1.7 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3390/galaxies9040115 | en_US |
dc.identifier.url | http://arxiv.org/abs/2112.03658v2 | en_US |
dc.identifier.url | https://www.mdpi.com/2075-4434/9/4/115 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 9 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 115 | 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 | GALAXIES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021arXiv211203658D | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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 | IRA Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
crisitem.author.orcid | 0000-0003-4120-9970 | - |
crisitem.author.orcid | 0000-0001-8121-6177 | - |
crisitem.author.orcid | 0000-0001-9143-6026 | - |
crisitem.author.orcid | 0000-0002-8627-6627 | - |
crisitem.author.orcid | 0000-0002-0375-8330 | - |
crisitem.author.orcid | 0000-0002-9087-2835 | - |
crisitem.author.orcid | 0000-0001-5544-0749 | - |
crisitem.journal.journalissn | 2075-4434 | - |
crisitem.journal.ance | E222261 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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D'Amato+21.pdf | PDF editoriale | 909.19 kB | Adobe PDF | View/Open |
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