Results 1 to 10 of about 1,075,291 (208)

The Origin and Evolution of Giant Radio Galaxies [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Giant radio galaxies are arguably the least understood of jetted active galactic nuclei (AGN). We propose that radio galaxies are the product of large mergers that do not involve radio galaxies or radio quasars, such as in merging spiral galaxies, while ...
David Garofalo
doaj   +5 more sources

Search and analysis of giant radio galaxies with associated nuclei (SAGAN)

open access: yesAstronomy & Astrophysics
Context. Giant radio galaxies (GRGs) represent the largest individual astrophysical structures, rivalling galaxy clusters in physical extent. Understanding how they attain such scales demands an examination of their large-scale cosmic surroundings ...
Mahato Mousumi   +4 more
doaj   +3 more sources

ENVIRONMENT DENSITY OF A GIANT RADIO STRUCTURE FOR GALAXIES AND QUASARS WITH STEEP RADIO SPECTRA [PDF]

open access: yesRadio Physics and Radio Astronomy, 2021
Purpose: Estimate of the environment density of giant (with the linear size of about megaparsec) radio structures for galaxies and quasars with steep low-frequency spectra taken from the UTR-2 catalogue. Study of the cosmological evolution of environment
A. P. Miroshnichenko
doaj   +1 more source

Viewing Classical Radio Galaxies with the Upgraded GMRT and MeerKAT—A Progress Report

open access: yesGalaxies, 2021
We present a progress report of a study of FR I and FR II radio galaxies. Several new morphological features in the radio emission are now revealed using the high (μJy) sensitivity reached in the range 550–1712 MHz, more than a factor of three, at the ...
Dharam V. Lal   +12 more
doaj   +1 more source

Cosmic ray acceleration to ultrahigh energy in radio galaxies [PDF]

open access: yesEPJ Web of Conferences, 2019
The origin of ultrahigh energy cosmic rays (UHECRs) is an open question. In this proceeding, we first review the general physical requirements that a source must meet for acceleration to 10-100 EeV, including the consideration that the shock is not ...
Matthews James H.   +3 more
doaj   +1 more source

Discovery of 178 Giant Radio Galaxies in 1059 deg2 of the Rapid ASKAP Continuum Survey at 888 MHz

open access: yesGalaxies, 2021
We report the results of a visual inspection of images of the Rapid ASKAP Continuum Survey (RACS) in search of extended radio galaxies (ERG) that reach or exceed linear sizes on the order of one Megaparsec. We searched a contiguous area of 1059 deg2 from
Heinz Andernach   +2 more
doaj   +1 more source

A Quick Look at the 3 GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey

open access: yesThe Astrophysical Journal Supplement Series, 2023
Active galactic nuclei (AGNs) can often be identified in radio images as two lobes, sometimes connected to a core by a radio jet. This multicomponent morphology unfortunately creates difficulties for source finders, leading to components that are (a ...
Yjan A. Gordon   +11 more
doaj   +1 more source

RELATIONS OF STRUCTURE COMPONENTS OF GIANT RADIO SOURCES

open access: yesOdessa Astronomical Publications, 2016
Our previous estimates of physical parameters of galaxies and quasars with steep radio spectrum have showed their great radio luminosity and giant radio structure.
A. P. Miroshnichenko
doaj   +1 more source

To the problem of the secondary CMB anisotropy separation

open access: yesEPJ Web of Conferences, 2016
We study contribution to the secondary anisotropy maps of cosmic microwave background (CMB) radiation which difficult to account for faint sources. Two effects are investigated.
Verkhodanov Oleg   +3 more
doaj   +1 more source

Relativistic jets in narrow-line Seyfert 1 galaxies. New discoveries and open questions

open access: yesEPJ Web of Conferences, 2013
Before the launch of the Fermi satellite only two classes of AGNs were known to produce relativistic jets and thus emit up to the γ-ray energy range: blazars and radio galaxies, both hosted in giant elliptical galaxies.
D’Ammando F.   +4 more
doaj   +1 more source

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