ChandraandHubble Space TelescopeObservations of Gamma‐Ray Blazars: Comparing Jet Emission at Small and Large Scales
Author(s) -
F. Tavecchio,
L. Maraschi,
A. Wolter,
C. C. Cheung,
R. M. Sambruna,
C. M. Urry
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/518085
Subject(s) - blazar , physics , astrophysics , jet (fluid) , astrophysical jet , bl lac object , scale (ratio) , gamma ray , astronomy , active galactic nucleus , galaxy , thermodynamics , quantum mechanics
We present new Chandra and HST data for four gamma-ray blazars selected on the basis of radio morphology with the aim of revealing X-ray and optical emission from their jets at large scales. All the sources have been detected. Spectral Energy Distributions of the large scale jets are obtained as well as new X-ray spectra for the blazar cores. Modeling for each object the core (sub-pc scale) and large-scale ({approx}> 100 kpc) jet SEDs, we derive the properties of the same jet at the two scales. The comparison of speeds and powers at different scales supports a simple scenario for the dynamics and propagation of high power relativistic jets
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