Probing the rapid formation of black holes and their Galaxy hosts in QSOs

Cutiva-Alvarez, Karla Alejandra; Coziol, Roger; Torres-Papaqui, Juan Pablo

doi:10.1093/mnras/stad675

Probing the rapid formation of black holes and their Galaxy hosts in QSOs

Journal Article · Mon Mar 06 00:00:00 EST 2023 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stad675· OSTI ID:2425261

Cutiva-Alvarez, Karla Alejandra ^[1]; Coziol, Roger ^[1]; Torres-Papaqui, Juan Pablo ^[1]

Univ. of Guanajuato (Mexico)

Using the modelling code x-cigale, we reproduced the spectral energy distributions (SEDs) of 1359 SDSS quasi-stellar objects (QSOs) within the redshift range 0 < z < 4, for which we have NIR/MIR fluxes with the highest quality and spectral data characterizing their supermassive black hole (SMBHs). Consistent with a rapid formation of the host galaxies, the star formation histories (SFHs) have small e-folding, at most 750 Myr using an SFH function for spiral or 1000 Myr using one for elliptical. Above z ∼ 1.6, the two solutions are degenerate, the SEDs being dominated by the active galactic nucleus (AGN) continuum and high star formation rates (SFRs), typical of starburst galaxies, while at lower redshifts the starburst nature of the host, independent from its morphology, is better reproduced by a spiral SFH. In general, the SFR increases with the redshift, the mass of the bulge, the AGN luminosity, and Eddington ratio, suggesting there is no evidence of AGN quenching of star formation. Comparing the specific BH accretion rate (BHAR) with specific SFR, all the QSOs at any redshift trace a linear sequence below the Eddington luminosity, in parallel and above the one-to-one relation, implying that QSOs are in a special phase of evolution during which the growth in mass of their SMBH is more rapid than the growth in mass of their galaxy hosts. This particular phase is consistent with a scenario where the galaxy hosts of QSOs in the past grew in mass more rapidly than their SMBHs, suggesting that a high star formation efficiency during their formation was responsible in limiting their masses.

View Accepted Manuscript (DOE)

Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)

Sponsoring Organization:: Consejo Nacional de Ciencia y Tecnología (CONACYT); Direccion de Apoyo a la Investigación y al Posgrado (DAIP); National Science Foundation (NSF); USDOE Office of Science (SC)

OSTI ID:: 2425261

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 521; ISSN 1365-2966; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging Finkelstein, Steven L.; Bagley, Micaela B.; Arrabal Haro, Pablo The Astrophysical Journal Letters, Vol. 940, Issue 2 https://doi.org/10.3847/2041-8213/ac966e	journal	December 2022
What do the Star Formation Histories of Galaxies tell us about the Starburst-AGN connection? Torres-Papaqui, J. P.; Coziol, R.; Plauchu-Frayn, I. arXiv https://doi.org/10.48550/arXiv.1308.1915	preprint	January 2013
A mid infrared study of low-luminosity AGNs with WISE Coziol, R.; Torres-Papaqui, J. P.; Plauchu-Frayn, I. arXiv https://doi.org/10.48550/arXiv.1405.4159	preprint	January 2014
Identification and properties of intense star-forming galaxies at redshifts z>10 Robertson, B. E.; Tacchella, S.; Johnson, B. D. arXiv https://doi.org/10.48550/arXiv.2212.04480	text	January 2022
Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2 Curtis-Lake, Emma; Carniani, Stefano; Cameron, Alex arXiv https://doi.org/10.48550/arXiv.2212.04568	preprint	January 2022
Quasars and Galaxy Formation Silk, Joseph; Rees, Martin J. arXiv https://doi.org/10.48550/arXiv.astro-ph/9801013	text	January 1998

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