Matches in SemOpenAlex for { <https://semopenalex.org/work/W2010633138> ?p ?o ?g. }
- W2010633138 abstract "A sample of 111 Fermi blazars each with a well-established radio core luminosity, broad-line luminosity, bolometric luminosity and black hole mass has been compiled from the literatures. We present a significant correlation between radio core and broad-line emission luminosities that supports a close link between accretion processes and relativistic jets. Analysis reveals a relationship of (mathrm{Log}mathrm{L}_{mathrm{BLR}}sim(0.81pm0.06)mathrm{Log} mathrm{L}_{mathrm{R}}^{mathrm{C}}) which is consistant with theoretical predicted coefficient and supports that blazar jets are powered by energy extraction from a rapidly spinning Kerr black hole through the magnetic field provided by the accretion disk. Through studying the correlation between the intrinsic bolometric luminosity and the black hole mass, we find a relationship of (mathrm{Log}frac{mathrm{L}_{mathrm{in}}}{mathrm{L}_{odot}}=(0.95pm0.26)mathrm{Log} frac{mathrm{M}}{mathrm{M}_{odot}}+(3.53pm2.24)) which supports mass-luminosity relation for Fermi blazars derived in this work is a powerlaw relation similar to that for main-sequence stars. Finally, EVOLUTIONARY SEQUENCE OF BLAZARS is discussed." @default.
- W2010633138 created "2016-06-24" @default.
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- W2010633138 date "2015-04-10" @default.
- W2010633138 modified "2023-10-17" @default.
- W2010633138 title "The jets-accretion relation, mass-luminosity relation in Fermi blazars" @default.
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- W2010633138 doi "https://doi.org/10.1007/s10509-015-2309-4" @default.
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