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DTIC ADA523212: Constraints on the Gamma-Ray Emitting Region in Bla... |
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by Defense Technical Information Center |
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Single-zone synchrotron self-Compton and external Compton |
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models are widely used to explain broadband Spectral |
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Energy Distributions (SEDs) of blazars from infrared to |
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gamma-rays. These models bear obvious similarities to the |
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homogeneous synchrotron cloud model which is often |
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applied to explain radio emission from individual |
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components of parsec-scale radio jets. The parsec-scale |
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core, typically the brightest and most compact feature of |
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blazar radio jet, could be the source of high-energy |
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emission. We report on ongoing work to test this |
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hypothesis by deriving the physical properties of parsec- |
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scale radio emitting regions of twenty bright Fermi |
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blazars using dedicated 5-43 GHz VLBA observations and |
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comparing these parameters to results of SED modeling. |
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Date Published: 2018-07-27 13:37:38 |
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Identifier: DTIC_ADA523212 |
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Item Size: 5916689 |
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Language: english |
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Media Type: texts |
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# Topics |
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DTIC Archive; ; MAX-PLANCK-INSTITUT F... |
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dticarchive |
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# Uploaded by |
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@chris85 |
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