We present new spectroscopic identifications of 12 X-shaped radio galaxies and use the spectral data to derive starburst histories and masses of the nuclear supermassive black holes in these galaxies. The observations were done with the 2.1-m telescope of the Observatorio Astronómico Nacional at San Pedro Mártir, México. The new spectroscopic results extend the sample of X-shaped radio galaxies studied with optical spectroscopy. We show that the combined sample of the X-shaped radio galaxies has statistically higher black-hole masses and older episodes of star formation than a control sample of canonical double-lobed radio sources with similar redshifts and luminosities. The data reveal enhanced star-formation activity in the X-shaped sa...
J2018-556, an X-shaped FR-I radio galaxy provides a unique opportunity to discuss the formation scen...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
With projects such as Laser Interferometer Space Antenna (LISA) and Pulsar Timing Arrays (PTAs) expe...
It has been suggested that the X-shaped morphology observed in some radio sources can reflect either...
A supermassive black hole binary may form during galaxy mergering. we investigate the interaction of...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
In the hierarchical galaxy formation model, today's galaxies are the product of frequent galaxy...
Coalescence of Supermassive Black Holes (SMBHs) in galaxy mergers is potentially the dominant contri...
International audienceWe use deep Herschel Space Observatory observations of a 90 per cent complete ...
Existing radio images of a few X-shaped radio galaxies reveal Z-symmetric morphologies in their weak...
The majority of radiation from galaxies containing active galactic nuclei (AGNs) is emitted not by t...
Abstract: We present results of an HI study of a complete sample of nearby radio galaxies. Our goal ...
Existing radio images of a few X-shaped radio galaxies reveal Z-symmetric morphologies in their weak...
We use neutral hydrogen (HI) and optical spectroscopic observations to compare the timescales of a m...
J2018-556, an X-shaped FR-I radio galaxy provides a unique opportunity to discuss the formation scen...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
With projects such as Laser Interferometer Space Antenna (LISA) and Pulsar Timing Arrays (PTAs) expe...
It has been suggested that the X-shaped morphology observed in some radio sources can reflect either...
A supermassive black hole binary may form during galaxy mergering. we investigate the interaction of...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
In the hierarchical galaxy formation model, today's galaxies are the product of frequent galaxy...
Coalescence of Supermassive Black Holes (SMBHs) in galaxy mergers is potentially the dominant contri...
International audienceWe use deep Herschel Space Observatory observations of a 90 per cent complete ...
Existing radio images of a few X-shaped radio galaxies reveal Z-symmetric morphologies in their weak...
The majority of radiation from galaxies containing active galactic nuclei (AGNs) is emitted not by t...
Abstract: We present results of an HI study of a complete sample of nearby radio galaxies. Our goal ...
Existing radio images of a few X-shaped radio galaxies reveal Z-symmetric morphologies in their weak...
We use neutral hydrogen (HI) and optical spectroscopic observations to compare the timescales of a m...
J2018-556, an X-shaped FR-I radio galaxy provides a unique opportunity to discuss the formation scen...
In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of s...
With projects such as Laser Interferometer Space Antenna (LISA) and Pulsar Timing Arrays (PTAs) expe...