We find a strong correlation between gamma-ray luminosity and Doppler factor for the detected sources. Within the BL Lac optical class, we find that high-synchrotron peaked BL Lacs have smaller Doppler factors, lower Lorentz factors, and larger angles to the line of sight than intermediate or low-synchrotron peaked BL Lacs. We use this intrinsic value to estimate Doppler factors for all 447 jets in our sample, and for the 309 jets with full kinematic information, we also estimate their Lorentz factors and angles to the line of sight. We use the observed median brightness temperatures combined with the measured jet kinematics to find a typical intrinsic Gaussian brightness temperature of 4.1 x 10^10 K, suggesting jet cores are at or below equipartition between particle and magnetic field energy in their median state. New Paper on Intrinsic Jet Properties: We have completed a new brightness temperature analysis of a sample of 447 AGN jets from the MOJAVE program. That is maintained by the MOJAVE team ( Lister Has made use of data from the MOJAVE database The following acknowledgment: "This research So we can add a link to the list of external If you are interested in Stokes Q,U,V (linearĪnd circular polarization) FITS images, please contactĭata in a publication, we ask that you please Gamma-ray emission detected by NASA's Fermi observator y.Īll calibrated (u,v) visibility and FITS data are available via html links Light-year scales, close to where they originate in theĪctive nucleus, and how this activity is correlated with Using these data to better understand the complexĮvolution and magnetic field structures of these jets on Headlights, as seen by an astronaut on the Moon). Polarization images with an angular resolution better thanġ milliarcsecond (the apparent separation of your car's Long Baseline Array (VLBA) at wavelengths of 7 mm,ġ.3 cm, and 2 cm, which enables us to make full World's highest resolution telescope: the Very Plasma moving nearly directly at us at speeds approaching Motions indicate that they contain highly energetic Material onto billion-solar-mass black holes located in These jets are powered by the accretion of These were observed from 1994-2002 as part of the VLBA 2Ĭm Survey. Polarization variations in jets associated with active Long-term program to monitor radio brightness and
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