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- W1645710063 abstract "Single-zone synchrotron self-Compton and external Compton models are widely used to explain broad-band Spectral Energy Distributions (SEDs) of blazars from infrared to gamma-rays. These models bear obvious similarities to the homogeneous synchrotron cloud model which is often applied to explain radio emission from individual components of parsec-scale radio jets. The parsec-scale core, typically the brightest and most compact feature of blazar radio jet, could be the source of high-energy emission. We report on ongoing work to test this hypothesis by deriving the physical properties of parsec-scale radio emitting regions of twenty bright Fermi blazars using dedicated 5-43 GHz VLBA observations and comparing these parameters to results of SED modeling." @default.
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- W1645710063 date "2010-06-15" @default.
- W1645710063 modified "2023-09-26" @default.
- W1645710063 title "Constraints on the gamma-ray emitting region in blazars from multi-frequency VLBI measurements" @default.
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- W1645710063 doi "https://doi.org/10.48550/arxiv.1006.3084" @default.
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