Add to ORKGInternational audienceThe optical synchrotron emission from extragalactic jets can be explained by the diffusive shock acceleration. But this process seems to be so efficient that the magnetic turbulences must be quite low. As to the origin of these turbulences, the interaction of the jet with the ISM may provide a common explanation for optical emission and one-sidedness of extragalactic jets
The dynamics and stability of extragalactic jets may be strongly influenced by small (and probable) ...
The extreme hypothesis that essentially all types of ultrarelativistic outflow - specifically AGN je...
We show that there is no universal law describing how the spectra and luminosity of synchrotron and ...
Abstract. We present a numerical model for electron acceler-ation and radiation inside the body of a...
Flattenings of nonthermal radiation spectra observed from knots and interknot locations of the jets ...
Freecomplete version on ADS:http://cdsads.u-strasbg.fr/cgi-bin/nph-data_query?bibcode=1992A%26A...25...
The observed emtsswns of radio waves from extragalactic radio jets are customarily interpreted in te...
Electromagnetic radiation from jets is normally considered to be incoherent synchrotron emission. So...
Full version with figures freely available on ADS at http://cdsads.u-strasbg.fr/cgi-bin/nph-iarticle...
Context. The central regions of galaxies are complex environments, rich in evolved and/or massive st...
Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Bec...
Nonthermal radiation observed from astrophysical systems containing relativistic jets and shocks, e....
It is generally accepted that relativistic jet outflows power the nonthermal emission from active g...
The dynamics and stability of extragalactic jets may be strongly influenced by small (and probable) ...
The extreme hypothesis that essentially all types of ultrarelativistic outflow - specifically AGN je...
We show that there is no universal law describing how the spectra and luminosity of synchrotron and ...
Abstract. We present a numerical model for electron acceler-ation and radiation inside the body of a...
Flattenings of nonthermal radiation spectra observed from knots and interknot locations of the jets ...
Freecomplete version on ADS:http://cdsads.u-strasbg.fr/cgi-bin/nph-data_query?bibcode=1992A%26A...25...
The observed emtsswns of radio waves from extragalactic radio jets are customarily interpreted in te...
Electromagnetic radiation from jets is normally considered to be incoherent synchrotron emission. So...
Full version with figures freely available on ADS at http://cdsads.u-strasbg.fr/cgi-bin/nph-iarticle...
Context. The central regions of galaxies are complex environments, rich in evolved and/or massive st...
Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Bec...
Nonthermal radiation observed from astrophysical systems containing relativistic jets and shocks, e....
It is generally accepted that relativistic jet outflows power the nonthermal emission from active g...
The dynamics and stability of extragalactic jets may be strongly influenced by small (and probable) ...
The extreme hypothesis that essentially all types of ultrarelativistic outflow - specifically AGN je...
We show that there is no universal law describing how the spectra and luminosity of synchrotron and ...