Results 1 to 10 of about 2,570 (146)

FIRST radio galaxy data set containing curated labels of classes FRI, FRII, compact and bent [PDF]

open access: yesData in Brief, 2023
Automated classification of astronomical sources is often challenging due to the scarcity of labelled training data. We present a data set with a total number of 2158 data items that contains radio galaxy images with their corresponding morphological ...
Florian Griese   +4 more
doaj   +2 more sources

Cosmic-Ray Acceleration and Magnetic Fields in Galaxy Clusters and Beyond: Insights from Radio Observations

open access: yesUniverse, 2023
The discovery of diffuse radio emission in galaxy clusters proved the existence of energetic cosmic-ray electrons and cosmic magnetic fields on Mpc-scales in the Universe.
Denis Wittor
doaj   +1 more source

The Dragonfly Galaxy. III. Jet Brightening of a High-redshift Radio Source Caught in a Violent Merger of Disk Galaxies

open access: yesThe Astrophysical Journal, 2023
The Dragonfly galaxy (MRC 0152-209), the most infrared-luminous radio galaxy at redshift z ∼ 2, is a merger system containing a powerful radio source and large displacements of gas.
Sophie Lebowitz   +10 more
doaj   +1 more source

Enigmatic Emission Structure around Mrk 783: Cross-Ionization of a Companion 100 kpc Away

open access: yesUniverse, 2023
Mrk 783 is a narrow-line Seyfert 1 galaxy that possesses a relatively large two-sided radio emission extending up to 14 kpc from the active nucleus possibly connected with a large-scale ionized gas emission. We obtained a deep [O iii] image that revealed
Alexei V. Moiseev   +2 more
doaj   +1 more source

The Dynamics of Radio Galaxies and Double–Double Radio Galaxies [PDF]

open access: yesJournal of Astrophysics and Astronomy, 2011
11 pages, 4 figures, Diffuse Radio Plasma Conference proceedings (held in Raman Research Institute, Bangalore, India)
Konar, C.   +6 more
openaire   +3 more sources

On the Encounter between the GASP Galaxy JO36 and the Radio Plume of GIN 049

open access: yesThe Astrophysical Journal, 2023
We report the serendipitous discovery of an unprecedented interaction between the radio lobe of a radio galaxy and a spiral galaxy. The discovery was made thanks to LOFAR observations at 144 MHz of the galaxy cluster A160 ( z = 0.04317) provided by the ...
Alessandro Ignesti   +17 more
doaj   +1 more source

The Interplay between Radio AGN Activity and Their Host Galaxies

open access: yesGalaxies, 2023
Radio activity in AGN (Active Galactic Nuclei) produce feedback on the host galaxy via the impact of the relativistic jets on the circumnuclear gas. Although radio jets can reach up to several times the optical radius of the host galaxy, in this review ...
Guilherme S. Couto   +1 more
doaj   +1 more source

RADIO DETECTION OF RADIO-QUIET GALAXIES [PDF]

open access: yesThe Astronomical Journal, 2008
We investigate the radio emission of ~185,000 quiescent (optically unclassifiable) galaxies selected from the Sloan Digital Sky Survey (SDSS). By median-stacking FIRST cutouts centered on the optically-selected sources, we are able to reach flux densities down to the 10s of microJy.
Hodge, J. A.   +3 more
openaire   +2 more sources

Powerful Yet Lonely: Is 3C 297 a High-redshift Fossil Group?

open access: yesThe Astrophysical Journal Supplement Series, 2022
The environment of the high-redshift ( z = 1.408), powerful radio-loud galaxy 3C 297 has several distinctive features of a galaxy cluster. Among them, a characteristic halo of hot gas revealed by Chandra X-ray observations.
Valentina Missaglia   +10 more
doaj   +1 more source

Radio galaxy zoo EMU: towards a semantic radio galaxy morphology taxonomy

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT We present a novel natural language processing (NLP) approach to deriving plain English descriptors for science cases otherwise restricted by obfuscating technical terminology. We address the limitations of common radio galaxy morphology classifications by applying this approach.
Micah Bowles   +22 more
openaire   +5 more sources

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