Add to ORKGThe infrared emission from the quasar 3C 48 has a luminosity L ≃ 5 x 10^(12) L_☉ and dominates the power output of the quasar system. It is shown that the infrared emission, unlike that of most radio-loud quasars, is most likely not an extension of the radio emission of the quasar. It is argued that the infrared emission in 3C 48 is probably thermal radiation arising in a highly luminous galaxy surrounding the quasar
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
The well-known quasar 3C48 is the most powerful compact steep-spectrum radio-loud QSO at low redshif...
The infrared emission from the quasar 3C 48 has a luminosity L ≃ 5 x 10^(12) L_☉ and dominates the p...
3C 318, a radio-loud quasar at z = 1.574, is a subgalactic-sized radio source, and a good test-bed f...
Measurements at 60 mu wavelength of 3CR quasars and powerful radio galaxies in the redshift range 0....
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We present near-infrared spectroscopy and imaging of the compact steep- spectrum radio source 3C 318...
Abstract. We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobe...
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We present the results of a programme of thermal-IR imaging of nineteen z~1 radio galaxies from the ...
Infrared Astronomical Satellite (IRAS) observations show that there is a maximum in the continuum en...
In order to test the unified scheme for luminous radio galaxies and quasars we observed 10 galaxy/qu...
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
The well-known quasar 3C48 is the most powerful compact steep-spectrum radio-loud QSO at low redshif...
The infrared emission from the quasar 3C 48 has a luminosity L ≃ 5 x 10^(12) L_☉ and dominates the p...
3C 318, a radio-loud quasar at z = 1.574, is a subgalactic-sized radio source, and a good test-bed f...
Measurements at 60 mu wavelength of 3CR quasars and powerful radio galaxies in the redshift range 0....
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We present near-infrared spectroscopy and imaging of the compact steep- spectrum radio source 3C 318...
Abstract. We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobe...
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-lo...
We present the results of a programme of thermal-IR imaging of nineteen z~1 radio galaxies from the ...
Infrared Astronomical Satellite (IRAS) observations show that there is a maximum in the continuum en...
In order to test the unified scheme for luminous radio galaxies and quasars we observed 10 galaxy/qu...
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
We present an analysis of the effects of luminosity on the shape of the mid-infrared spectral energy...
The well-known quasar 3C48 is the most powerful compact steep-spectrum radio-loud QSO at low redshif...
