We report multi-frequency observations of large radio galaxies 3C 35 and 3C 284. The low-frequency observations were done with Giant Metrewave Radio Telescope starting from $\sim$150 MHz, and the high-frequency observations were done with the Very Large Array. We have studied the radio morphology of these two sources at different frequencies. We present the spectral ageing map using two of the most widely used models, the Kardashev-Pacholczyk and Jaffe-Perola models. Another more realistic and complex Tribble model is also used. We also calculate the jet-power and the speed of the radio lobes of these galaxies. We check for whether any episodic jet activity is present or not in these galaxies and found no sign of such kind of activity.Comme...
In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasa...
Radio-loud AGN represent the most energetic and influential large-scale structures in the Universe. ...
I present four-frequency radio observations of the wide-angle tail radio galaxy 3C130. By a techniqu...
We report multi-frequency observations of large radio galaxies 3C 35 and 3C 284. The low-frequency o...
Received; accepted Aims. Radio galaxies with a projected linear size & 1 Mpc are classified as g...
10 pages, 6 figuresWe have examined the giant radio galaxy 3C~236 using LOFAR at 143 MHz down to an ...
We have examined the giant radio galaxy 3C 236 using LOFAR at 143 MHz down to an angular resolution ...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Recent investigations have shown that many parameters and assumptions made in the application of spe...
© ESO 2020. The original publication is available at https://doi.org/10.1051/0004-6361/202037457.Con...
We have formed a complete sample of 26 low redshift (z less than or similar to 0.3) giant radio gala...
The original article can be found at: http://www3.interscience.wiley.com Copyright Blackwell Publish...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasa...
Radio-loud AGN represent the most energetic and influential large-scale structures in the Universe. ...
I present four-frequency radio observations of the wide-angle tail radio galaxy 3C130. By a techniqu...
We report multi-frequency observations of large radio galaxies 3C 35 and 3C 284. The low-frequency o...
Received; accepted Aims. Radio galaxies with a projected linear size & 1 Mpc are classified as g...
10 pages, 6 figuresWe have examined the giant radio galaxy 3C~236 using LOFAR at 143 MHz down to an ...
We have examined the giant radio galaxy 3C 236 using LOFAR at 143 MHz down to an angular resolution ...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Recent investigations have shown that many parameters and assumptions made in the application of spe...
© ESO 2020. The original publication is available at https://doi.org/10.1051/0004-6361/202037457.Con...
We have formed a complete sample of 26 low redshift (z less than or similar to 0.3) giant radio gala...
The original article can be found at: http://www3.interscience.wiley.com Copyright Blackwell Publish...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasa...
Radio-loud AGN represent the most energetic and influential large-scale structures in the Universe. ...
I present four-frequency radio observations of the wide-angle tail radio galaxy 3C130. By a techniqu...