Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30702
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Matsuoka, K. | en_US |
dc.contributor.author | Toba, Y. | en_US |
dc.contributor.author | Shidatsu, M. | en_US |
dc.contributor.author | Ueda, Y. | en_US |
dc.contributor.author | Iwasawa, K. | en_US |
dc.contributor.author | Terashima, Y. | en_US |
dc.contributor.author | Imanishi, M. | en_US |
dc.contributor.author | Nagao, T. | en_US |
dc.contributor.author | Marconi, Alessandro | en_US |
dc.contributor.author | Wang, W. -H. | en_US |
dc.date.accessioned | 2021-03-15T12:23:38Z | - |
dc.date.available | 2021-03-15T12:23:38Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30702 | - |
dc.description.abstract | We present a near-infrared (NIR) spectrum of WISE J104222.11+164115.3, an extremely red dust-obscured galaxy (DOG), which has been observed with the Long-slit Intermediate Resolution Infrared Spectrograph (LIRIS) on the 4.2m William Hershel Telescope. This object was selected as a hyper-luminous DOG candidate at z ∼ 2 by combining the optical and IR photometric data based on the Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE), although its redshift had not yet been confirmed. Based on the LIRIS observation, we confirmed its redshift of 2.521 and total IR luminosity of log(L<SUB>IR</SUB>/L<SUB>☉</SUB>) = 14.57, which satisfies the criterion for an extremely luminous IR galaxy (ELIRG). Moreover, we indicate that this object seems to have an extremely massive black hole with M<SUB>BH</SUB> = 10<SUP>10.92</SUP> M<SUB>☉</SUB> based on the broad Hα line: the host stellar mass is derived as M<SUB>⋆</SUB> = 10<SUP>13.55</SUP> M<SUB>☉</SUB> by a fit of the spectral energy distribution. Very recently, it has been reported that this object is an anomalous gravitationally lensed quasar based on near-IR high-resolution imaging data obtained with the Hubble Space Telescope. Its magnification factor has also been estimated with some uncertainty (i.e., μ = 53-122). We investigate the ratio of the black hole to galaxy mass, which is less strongly affected by a lensing magnification factor, instead of the absolute values of the luminosities and masses. We find that the M<SUB>BH</SUB>/M<SUB>⋆</SUB> ratio (i.e., 0.0140-0.0204) is significantly higher than the local relation, following a sequence of unobscured quasars instead of obscured objects (e.g., submillimeter galaxies) at the same redshift. Moreover, the LIRIS spectrum shows strongly blueshifted oxygen lines with an outflowing velocity of ∼1100 km s<SUP>-1</SUP>, and our Swift X-ray observation also supports that this source is an absorbed AGN with an intrinsic column density of N<SUB>H</SUB><SUP>int</SUP> = 4.9 × 10<SUP>23</SUP> cm<SUP>-2</SUP>. These results imply that WISE J104222.11+164115.3 is in a blow-out phase at the end of the buried rapid black hole growth. | en_US |
dc.language.iso | eng | en_US |
dc.title | Ratio of black hole to galaxy mass of an extremely red dust-obscured galaxy at z = 2.52 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201833943 | en_US |
dc.identifier.scopus | 2-s2.0-85058015103 | en_US |
dc.identifier.isi | 000452392900001 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2018/12/aa33943-18/aa33943-18.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 620 | en_US |
dc.relation.firstpage | L3 | 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 | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018A&A...620L...3M | 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::PE9_8 Formation and evolution of galaxies | 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 | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-9889-4238 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
aa33943-18.pdf | PDF editoriale | 606.1 kB | Adobe PDF | Visualizza/apri |
Page view(s)
65
controllato il 20-lug-2024
Download(s)
12
controllato il 20-lug-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.