Matches in SemOpenAlex for { <https://semopenalex.org/work/W3162477646> ?p ?o ?g. }
- W3162477646 endingPage "5211" @default.
- W3162477646 startingPage "5192" @default.
- W3162477646 abstract "Here we consider the perspective to detect sub-pc super-massive binary black-hole (SMBBH) systems using long-term photometric and spectroscopic monitoring campaigns of active galactic nuclei. This work explores the nature of long-term spectral variability caused by the dynamical effects of SMBBH systems. We describe in great detail a model of SMBBH system which considers that both black holes have their accretion disc and additional line emitting region(s). We simulate the H$beta$ spectral band (continuum+broad H$beta$ line) for different mass ratios of components and different total masses of the SMBBH systems ($10^6-10^8mathrm{Modot}$). We analyze the set of continuum and broad line light curves for several full orbits of SMBBHs with different parameters, to test the possibility to extract the periodicity of the system. We consider different levels of the signal-to-noise ratio, which is added to the simulated spectra. Our analysis showed that the continuum and broad line profiles emitted from an SMBBH system are strongly dependent, not only on the mass ratio of the components but also on the total mass of the system. We found that the mean broad line profile and its rms could indicate the presence of an SMBBH. However, some effects caused by the dynamics of a binary system could be hidden due to a low signal-to-noise ratio. Finally, we can conclude that the long-term AGN monitoring campaigns could be beneficial for the detection of SMBBH candidates." @default.
- W3162477646 created "2021-05-24" @default.
- W3162477646 creator A5009513108 @default.
- W3162477646 creator A5047891641 @default.
- W3162477646 creator A5061866689 @default.
- W3162477646 creator A5079679564 @default.
- W3162477646 date "2021-05-27" @default.
- W3162477646 modified "2023-10-11" @default.
- W3162477646 title "Detecting subparsec supermassive binary black holes: Long-term monitoring perspective" @default.
- W3162477646 cites W1468711679 @default.
- W3162477646 cites W1581797844 @default.
- W3162477646 cites W1781203010 @default.
- W3162477646 cites W1965140082 @default.
- W3162477646 cites W1972394604 @default.
- W3162477646 cites W1974618482 @default.
- W3162477646 cites W1986316936 @default.
- W3162477646 cites W1991074096 @default.
- W3162477646 cites W1995061453 @default.
- W3162477646 cites W1995843220 @default.
- W3162477646 cites W2011739082 @default.
- W3162477646 cites W2016491898 @default.
- W3162477646 cites W2028382975 @default.
- W3162477646 cites W2036919467 @default.
- W3162477646 cites W2061815116 @default.
- W3162477646 cites W2068728750 @default.
- W3162477646 cites W2072944399 @default.
- W3162477646 cites W2080259092 @default.
- W3162477646 cites W2103474895 @default.
- W3162477646 cites W2105041115 @default.
- W3162477646 cites W2108389059 @default.
- W3162477646 cites W2116046246 @default.
- W3162477646 cites W2127664311 @default.
- W3162477646 cites W2129433901 @default.
- W3162477646 cites W2147925360 @default.
- W3162477646 cites W2150157686 @default.
- W3162477646 cites W2266202083 @default.
- W3162477646 cites W2287952050 @default.
- W3162477646 cites W2410197117 @default.
- W3162477646 cites W2439892847 @default.
- W3162477646 cites W2574682548 @default.
- W3162477646 cites W2587587706 @default.
- W3162477646 cites W2604166262 @default.
- W3162477646 cites W2773409868 @default.
- W3162477646 cites W2892282539 @default.
- W3162477646 cites W2898179605 @default.
- W3162477646 cites W2902466147 @default.
- W3162477646 cites W2917331530 @default.
- W3162477646 cites W2951704600 @default.
- W3162477646 cites W3005861934 @default.
- W3162477646 cites W3010711607 @default.
- W3162477646 cites W3033957135 @default.
- W3162477646 cites W3086628218 @default.
- W3162477646 cites W3098035876 @default.
- W3162477646 cites W3098492522 @default.
- W3162477646 cites W3098725709 @default.
- W3162477646 cites W3099028325 @default.
- W3162477646 cites W3099085724 @default.
- W3162477646 cites W3099716756 @default.
- W3162477646 cites W3099839151 @default.
- W3162477646 cites W3100000149 @default.
- W3162477646 cites W3100124715 @default.
- W3162477646 cites W3100486880 @default.
- W3162477646 cites W3101090931 @default.
- W3162477646 cites W3101144359 @default.
- W3162477646 cites W3101187446 @default.
- W3162477646 cites W3102048068 @default.
- W3162477646 cites W3104106231 @default.
- W3162477646 cites W3104720823 @default.
- W3162477646 cites W3104797732 @default.
- W3162477646 cites W3105001641 @default.
- W3162477646 cites W3105007371 @default.
- W3162477646 cites W3105089311 @default.
- W3162477646 cites W3105175759 @default.
- W3162477646 cites W3105873562 @default.
- W3162477646 cites W3106056607 @default.
- W3162477646 cites W3106537294 @default.
- W3162477646 cites W3115647240 @default.
- W3162477646 cites W3124048289 @default.
- W3162477646 cites W3124507325 @default.
- W3162477646 cites W3124960205 @default.
- W3162477646 doi "https://doi.org/10.1093/mnras/stab1510" @default.
- W3162477646 hasPublicationYear "2021" @default.
- W3162477646 type Work @default.
- W3162477646 sameAs 3162477646 @default.
- W3162477646 citedByCount "4" @default.
- W3162477646 countsByYear W31624776462021 @default.
- W3162477646 countsByYear W31624776462022 @default.
- W3162477646 crossrefType "journal-article" @default.
- W3162477646 hasAuthorship W3162477646A5009513108 @default.
- W3162477646 hasAuthorship W3162477646A5047891641 @default.
- W3162477646 hasAuthorship W3162477646A5061866689 @default.
- W3162477646 hasAuthorship W3162477646A5079679564 @default.
- W3162477646 hasBestOaLocation W31624776462 @default.
- W3162477646 hasConcept C121332964 @default.
- W3162477646 hasConcept C1276947 @default.
- W3162477646 hasConcept C173120059 @default.
- W3162477646 hasConcept C182283691 @default.
- W3162477646 hasConcept C188232333 @default.