Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies
We present an improved study of the relation between supermassive black hole growth and their host galaxy properties in the local Universe (z < 0.33). To this end, we build an extensive sample combining spectroscopic measurements of star formation rate (SFR) and stellar mass from Sloan Digital Sk...
| Autores: | , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Universidad de Cantabria (UC) |
| Repositorio: | UCrea Repositorio Abierto de la Universidad de Cantabria |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.unican.es:10902/34258 |
| Acceso en línea: | https://hdl.handle.net/10902/34258 |
| Access Level: | acceso abierto |
| Palabra clave: | Accretion, accretion discs Galaxies: active Galaxies: elliptical and lenticular, cD Galaxies: spiral Galaxies: star formation X-rays: galaxies |
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Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxiesTorbaniuk, O.Paolillo, M.D'Abrusco, R.Vignali. C.Georgakakis, A.Carrera Troyano, Francisco Jesús|||0000-0003-2135-9023Civano, F.Accretion, accretion discsGalaxies: activeGalaxies: elliptical and lenticular, cDGalaxies: spiralGalaxies: star formationX-rays: galaxiesWe present an improved study of the relation between supermassive black hole growth and their host galaxy properties in the local Universe (z < 0.33). To this end, we build an extensive sample combining spectroscopic measurements of star formation rate (SFR) and stellar mass from Sloan Digital Sky Survey, with specific Black Hole accretion rate (sBHAR, λsBHAR ∝ Lx/M∗) derived from the XMM–Newton Serendipitous Source Catalogue (3XMM–DR8) and the Chandra Source Catalogue (CSC2.0). We find that the sBHAR probability distribution for both star-forming and quiescent galaxies has a power-law shape peaking at log λsBHAR ∼ −3.5 and declining towards lower sBHAR in all stellar mass ranges. This finding confirms the decrease of active galactic nucleus (AGN) activity in the local Universe compared to higher redshifts. We observe a significant correlation between log λsBHAR and log SFR in almost all stellar mass ranges, but the relation is shallower compared to higher redshifts, indicating a reduced availability of accreting material in the local Universe. At the same time, the BHAR-to-SFR ratio for star-forming galaxies strongly correlates with stellar mass, supporting the scenario where both AGN activity and stellar formation primarily depend on the stellar mass via fuelling by a common gas reservoir. Conversely, this ratio remains constant for quiescent galaxies, possibly indicating the existence of the different physical mechanisms responsible for AGN fuelling or different accretion mode in quiescent galaxies.OT and MP acknowledge the financial contribution from the agreement ASI-INAF n.2017-14-H.O. and from PRIN-MIUR 2022 funded by the European Union – Next Generation EU. MP also acknowledges support from the Timedomes grant within the ‘INAF 2023 Finanziamento della Ricerca Fondamentale’. AG acknowledges support from the EU H2020-MSCA-ITN-2019 Project 860744 ‘BiD4BESt: Big Data applications for Black hole Evolution Studies’14 and the Hellenic Foundation for Research and Innovation (HFRI) project ‘4MOVE-U’ grant agreement 2688, which is part of the programme 2nd Call for HFRI Research Projects to support Faculty Members and Researchers’. FJC acknowledges support from the grant PID2021-122955OB-C41 funded by MCIN/AEI/10.13039/501100011033 and by ERDF A way of making Europe.Oxford University PressUniversidad de Cantabria20242024-02-01journal articlehttp://purl.org/coar/resource_type/c_6501NAhttp://purl.org/coar/version/c_be7fb7dd8ff6fe43info:eu-repo/semantics/articlehttps://hdl.handle.net/10902/34258Monthly Notices of the Royal Astronomical Society, 2024, 527(4), 12091-12108reponame:UCrea Repositorio Abierto de la Universidad de Cantabriainstname:Universidad de Cantabria (UC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.unican.es:10902/342582026-06-02T12:39:31Z |
| dc.title.none.fl_str_mv |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| title |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| spellingShingle |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies Torbaniuk, O. Accretion, accretion discs Galaxies: active Galaxies: elliptical and lenticular, cD Galaxies: spiral Galaxies: star formation X-rays: galaxies |
| title_short |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| title_full |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| title_fullStr |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| title_full_unstemmed |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| title_sort |
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies |
| dc.creator.none.fl_str_mv |
Torbaniuk, O. Paolillo, M. D'Abrusco, R. Vignali. C. Georgakakis, A. Carrera Troyano, Francisco Jesús|||0000-0003-2135-9023 Civano, F. |
| author |
Torbaniuk, O. |
| author_facet |
Torbaniuk, O. Paolillo, M. D'Abrusco, R. Vignali. C. Georgakakis, A. Carrera Troyano, Francisco Jesús|||0000-0003-2135-9023 Civano, F. |
| author_role |
author |
| author2 |
Paolillo, M. D'Abrusco, R. Vignali. C. Georgakakis, A. Carrera Troyano, Francisco Jesús|||0000-0003-2135-9023 Civano, F. |
| author2_role |
author author author author author author |
| dc.contributor.none.fl_str_mv |
Universidad de Cantabria |
| dc.subject.none.fl_str_mv |
Accretion, accretion discs Galaxies: active Galaxies: elliptical and lenticular, cD Galaxies: spiral Galaxies: star formation X-rays: galaxies |
| topic |
Accretion, accretion discs Galaxies: active Galaxies: elliptical and lenticular, cD Galaxies: spiral Galaxies: star formation X-rays: galaxies |
| description |
We present an improved study of the relation between supermassive black hole growth and their host galaxy properties in the local Universe (z < 0.33). To this end, we build an extensive sample combining spectroscopic measurements of star formation rate (SFR) and stellar mass from Sloan Digital Sky Survey, with specific Black Hole accretion rate (sBHAR, λsBHAR ∝ Lx/M∗) derived from the XMM–Newton Serendipitous Source Catalogue (3XMM–DR8) and the Chandra Source Catalogue (CSC2.0). We find that the sBHAR probability distribution for both star-forming and quiescent galaxies has a power-law shape peaking at log λsBHAR ∼ −3.5 and declining towards lower sBHAR in all stellar mass ranges. This finding confirms the decrease of active galactic nucleus (AGN) activity in the local Universe compared to higher redshifts. We observe a significant correlation between log λsBHAR and log SFR in almost all stellar mass ranges, but the relation is shallower compared to higher redshifts, indicating a reduced availability of accreting material in the local Universe. At the same time, the BHAR-to-SFR ratio for star-forming galaxies strongly correlates with stellar mass, supporting the scenario where both AGN activity and stellar formation primarily depend on the stellar mass via fuelling by a common gas reservoir. Conversely, this ratio remains constant for quiescent galaxies, possibly indicating the existence of the different physical mechanisms responsible for AGN fuelling or different accretion mode in quiescent galaxies. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024 2024-02-01 |
| dc.type.none.fl_str_mv |
journal article http://purl.org/coar/resource_type/c_6501 NA http://purl.org/coar/version/c_be7fb7dd8ff6fe43 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/10902/34258 |
| url |
https://hdl.handle.net/10902/34258 |
| dc.language.none.fl_str_mv |
Inglés eng |
| language_invalid_str_mv |
Inglés |
| language |
eng |
| dc.rights.none.fl_str_mv |
open access http://purl.org/coar/access_right/c_abf2 Attribution 4.0 International http://creativecommons.org/licenses/by/4.0/ |
| dc.rights.openaire.fl_str_mv |
info:eu-repo/semantics/openAccess |
| rights_invalid_str_mv |
open access http://purl.org/coar/access_right/c_abf2 Attribution 4.0 International http://creativecommons.org/licenses/by/4.0/ |
| eu_rights_str_mv |
openAccess |
| dc.publisher.none.fl_str_mv |
Oxford University Press |
| publisher.none.fl_str_mv |
Oxford University Press |
| dc.source.none.fl_str_mv |
Monthly Notices of the Royal Astronomical Society, 2024, 527(4), 12091-12108 reponame:UCrea Repositorio Abierto de la Universidad de Cantabria instname:Universidad de Cantabria (UC) |
| instname_str |
Universidad de Cantabria (UC) |
| reponame_str |
UCrea Repositorio Abierto de la Universidad de Cantabria |
| collection |
UCrea Repositorio Abierto de la Universidad de Cantabria |
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1869414331113799680 |
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15,811543 |