Exploring the X-ray universe via timing: mass of the active galactic nucleus black hole XMMUJ134736.6+173403
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00552767" target="_blank" >RIV/67985815:_____/21:00552767 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921320003312" target="_blank" >http://dx.doi.org/10.1017/S1743921320003312</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921320003312" target="_blank" >10.1017/S1743921320003312</a>
Alternative languages
Result language
angličtina
Original language name
Exploring the X-ray universe via timing: mass of the active galactic nucleus black hole XMMUJ134736.6+173403
Original language description
A strong quasi-periodic modulation has recently been revealed in the X-ray flux of the X-ray source XMMUJ134736.6+173403. The two observed twin-peak quasiperiodic oscillations (QPOs) exhibit a 3:1 frequency ratio and strongly support the evidence for the presence of an active galactic nucleus black hole (AGN BH). It has been suggested that detections of twin-peak QPOs with commensurable frequency ratios and scaling of their periods with BH mass could provide the basis for a method intended to determine the mass of BH sources, such as AGNs. Assuming the orbital origin of QPOs, we calculate the upper and lower limit on the AGN BH mass M, reaching M ≍ 107-109 M⊙. Compared to mass estimates of other sources, XMMUJ134736.6+173403 appears to be the most massive source with commensurable QPO frequencies, and its mass represents the current observational upper limit on the AGN BH mass obtained from the QPO observations.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Nuclear Activity in Galaxies Across Cosmic Time
ISBN
9781108492010
ISSN
1743-9213
e-ISSN
1743-9221
Number of pages
3
Pages from-to
348-350
Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Addis Ababa
Event date
Oct 7, 2019
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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