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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierQABCDSTQQW/46AC8EL
Repositoryurlib.net/www/2022/02.03.21.48
Last Update2022:02.03.21.48.33 (UTC) simone
Metadata Repositoryurlib.net/www/2022/02.03.21.48.33
Metadata Last Update2023:01.03.16.46.29 (UTC) administrator
DOI10.1093/mnras/stab3414
ISSN0035-8711
1365-2966
Citation KeyPrietoRodrPandMari:2022:NoBlHo
TitleA novel black hole mass scaling relation based on coronal gas, and its dependence with the accretion disc
Year2022
MonthFeb.
Access Date2024, May 13
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2477 KiB
2. Context
Author1 Prieto, Almudena
2 Rodriguez-Ardilla, Alberto
3 Panda, Swayamtrupta
4 Marinello, Murilo
ORCID1 0000-0002-3585-2639
Group1
2 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidad de La Laguna
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Polish Academy of Sciences
4 Laboratório Nacional de Astrofísica (LNA)
Author e-Mail Address1 aprieto@iac.es
JournalMonthly Notices of the Royal Astronomical Society
Volume510
Number1
Pages1010-1030
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2022-02-03 21:48:33 :: simone -> administrator ::
2022-02-03 21:48:34 :: administrator -> simone :: 2022
2022-02-03 21:49:40 :: simone -> administrator :: 2022
2023-01-03 16:46:29 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsaccretion
accretion discs
radiation mechanism thermal
techniques: spectroscopic
galaxies: active
quasars: emission lines
AbstractUsing bona-fide black hole (BH) mass estimates from reverberation mapping and the line ratio [Si VI] 1.963 mu m/Br gamma(broad) as tracer of the AGN ionizing continuum, a novel BH-mass scaling relation of the form log(M-BH) = (6.40 +/- 0.17) - (1.99 +/- 0.37) x log ([Si VI]/Br gamma(broad)), dispersion 0.47 dex, over the BH mass interval, 10(6)-10(8) M-circle dot is found. Following on the geometrically thin accretion disc approximation and after surveying a basic parameter space for coronal lines production, we believe one of main drivers of the relation is the effective temperature of the disc, which is effectively sampled by the [Si VI] 1.963 mu m coronal line for the range of BH masses considered. By means of CLOUDY photoionization models, the observed anticorrelation appears to be formally in line with the thin disc prediction T-di(sc) proportional to M-BH(-1/4).
AreaCEA
Arrangementurlib.net > Produção a partir de 2021 > CGCE > A novel black...
doc Directory Contentaccess
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/QABCDSTQQW/46AC8EL
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/QABCDSTQQW/46AC8EL
Languageen
Target FilePrieto_2022_novel.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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