dc.contributor.author | Carrera, F. J. | |
dc.contributor.author | Page, M. J. | |
dc.contributor.author | Stevens, J. A. | |
dc.contributor.author | Ivison, R. J. | |
dc.contributor.author | Dwelly, T. | |
dc.contributor.author | Ebrero, J. | |
dc.contributor.author | Falocco, S. | |
dc.date.accessioned | 2013-01-07T16:29:15Z | |
dc.date.available | 2013-01-07T16:29:15Z | |
dc.date.issued | 2011-06 | |
dc.identifier.citation | Carrera , F J , Page , M J , Stevens , J A , Ivison , R J , Dwelly , T , Ebrero , J & Falocco , S 2011 , ' A strongly star-forming group : three massive galaxies associated with a quasi-stellar object ' , Monthly Notices of the Royal Astronomical Society , vol. 413 , no. 4 , pp. 2791-2807 . https://doi.org/10.1111/j.1365-2966.2011.18352.x | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | ORCID: /0000-0002-4010-8310/work/62747622 | |
dc.identifier.uri | http://hdl.handle.net/2299/9500 | |
dc.description | The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Society | |
dc.description.abstract | We present here photometric redshift confirmation of the presence of large-scale structure around the z = 1.82 quasi-stellar object (QSO) RX J0941, which shows an overdensity of submillimetre (submm) sources. Radio imaging confirms the presence of the submm sources and pinpoints their likely optical near-infrared (NIR) counterparts. Four of the five submm sources present in this field (including the QSO) have counterparts with redshifts compatible with z = 1.82. We show that our photometric redshifts are robust against the use of different spectral templates. We have measured the galaxy stellar mass of the submm galaxies from their rest-frame K-band luminosity obtaining log(M-*/M-circle dot) similar to 11.5 +/- 0.2, slightly larger than the Schechter mass of present-day galaxies, and hence indicating that most of the stellar mass is already formed. We present optical-to-radio spectral energy distributions (SEDs) of the five Submillimetre Common-User Bolometer Array (SCUBA) sources. The emission of RX J0941 is dominated by reprocessed active galactic nucleus (AGN) emission in the observed mid-IR (MIR) range, while the starburst contribution completely dominates in the submm range. The SEDs of the other three counterparts are compatible with a dominant starburst contribution above similar to 24 mu m, with star formation rates similar to 2000 M-circle dot yr-1, central dust masses log(M-dust/M-circle dot) similar to 9 +/- 0.5 and hence central gas masses log(M-gas/M-circle dot) similar to 10.7. There is very little room for an AGN contribution. From X-ray upper limits and the observed 24 mu m flux, we derive a maximum 2-10 keV X-ray luminosity of 1044 erg s-1 for any putative AGN, even if they are heavily obscured. This in turn points to relatively small black holes with log(M-center dot/M-circle dot) less than or similar to 8 and hence stellar-to-black hole mass ratios about 1 order of magnitude higher than those observed in the present Universe: most of their central black hole masses are still to be accreted. Local stellar-to-black hole mass ratios can be reached if similar to 1.3 per cent of the available nuclear gas mass is accreted. | en |
dc.format.extent | 17 | |
dc.format.extent | 1303644 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.subject | galaxies: evolution | |
dc.subject | galaxies: formation | |
dc.subject | galaxies: high-redshift | |
dc.subject | galaxies: starburst | |
dc.title | A strongly star-forming group : three massive galaxies associated with a quasi-stellar object | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Science & Technology Research Institute | |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1111/j.1365-2966.2011.18352.x | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |