Abstract
We report on an analysis of intrinsic jet properties between sources
detected by the Fermi Gamma-ray Space Telescope during its first three
months of science operations and those not detected in a sample 62
blazars. By combining high-resolution VLBI images and
millimetre-wavelength flux density monitoring data, we have estimated
their jet Doppler factors, Lorentz factors, and viewing angles in the
observer’s frame and in the frame comoving with the jet. The
analysis shows that, in addition to having on average higher variability
Doppler factors, the blazars detected by the Fermi have a distribution
of comoving frame viewing angles that is significantly narrower than
that of the γ-ray weak blazars and centred roughly perpendicular
to the jet axis. The lack of γ-ray bright blazars at small
comoving frame viewing angles hints that their γ-ray emission may
be intrinsically anisotropic or depend on the Lorentz factor.
Original language | English |
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Title of host publication | Accretion and Ejection in AGN: a Global View |
Subtitle of host publication | Proceedings of a workshop held June 22-26, 2009 in Como, Italy |
Editors | Laura Maraschi, Gabriele Ghisellini, Roberto Della Ceca, Fabrizio Tavecchio |
Publisher | Astronomical Society of the Pacific |
Pages | 306-307 |
ISBN (Electronic) | 978-1-58381-735-3 |
ISBN (Print) | 978-1-58381-734-6 |
Publication status | Published - 2010 |
MoE publication type | B3 Non-refereed conference publication |
Event | Conference on Accretion and Ejection in AGN: A Global View - Como, Italy Duration: 22 Jun 2009 → 26 Jun 2009 |
Publication series
Name | Astronomical society of the pacific Conference Series |
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Publisher | Astronomical Society of the Pacific |
Volume | 427 |
ISSN (Print) | 1050-3390 |
Conference
Conference | Conference on Accretion and Ejection in AGN: A Global View |
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Country/Territory | Italy |
City | Como |
Period | 22/06/2009 → 26/06/2009 |
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Metsähovi Radio Observatory
Tammi, J. (Manager)
School of Electrical EngineeringFacility/equipment: Facility