Fermi/non-Fermi blazars jet power and accretion

DOI

We study the relationship between jet power and accretion for Fermi and non-Fermi blazars. We also compare the relevant parameter. Our main results are: (i) Fermi and non-Fermi blazars have significant differences in red shift, black hole mass and broad line luminosity. (ii) Fermi blazars have a higher average core-dominance parameter than non-Fermi blazars, which suggests that Fermi blazars have a strong beaming effect. (iii) We find a significant correlation between broad line emission and jet power for Fermi and non-Fermi blazars, which suggests a direct tight connection between jet and accretion. (iv) The accretion and black hole mass may have a different contribution to jet power for Fermi and non-Fermi blazars.

Cone search capability for table J/MNRAS/451/4193/table2 (The Fermi blazars)

Cone search capability for table J/MNRAS/451/4193/table3 (The non-Fermi blazars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74514193
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/451/4193
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/451/4193
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/451/4193
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/451/4193
Provenance
Creator Chen Y.Y.; Zhang X.; Zhang H.J.; Yu X.L.
Publisher CDS
Publication Year 2018
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; High Energy Astrophysics; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy