z-logo
open-access-imgOpen Access
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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom