Abstrakti
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.
Alkuperäiskieli | Englanti |
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Otsikko | Accretion and Ejection in AGN: a Global View |
Alaotsikko | Proceedings of a workshop held June 22-26, 2009 in Como, Italy |
Toimittajat | Laura Maraschi, Gabriele Ghisellini, Roberto Della Ceca, Fabrizio Tavecchio |
Kustantaja | Astronomical Society of the Pacific |
Sivut | 306-307 |
ISBN (elektroninen) | 978-1-58381-735-3 |
ISBN (painettu) | 978-1-58381-734-6 |
Tila | Julkaistu - 2010 |
OKM-julkaisutyyppi | B3 Vertaisarvioimaton artikkeli konferenssijulkaisussa |
Tapahtuma | Conference on Accretion and Ejection in AGN: A Global View - Como, Italia Kesto: 22 kesäk. 2009 → 26 kesäk. 2009 |
Julkaisusarja
Nimi | Astronomical society of the pacific Conference Series |
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Kustantaja | Astronomical Society of the Pacific |
Vuosikerta | 427 |
ISSN (painettu) | 1050-3390 |
Conference
Conference | Conference on Accretion and Ejection in AGN: A Global View |
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Maa/Alue | Italia |
Kaupunki | Como |
Ajanjakso | 22/06/2009 → 26/06/2009 |
Sormenjälki
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