Results 1 to 10 of about 25,768 (176)

‘Normal’ Fanaroff-Riley type II radio galaxies as a probe of the nature of X-shaped radio sources [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2008
We present a multiwavelength radio study of a sample of nearby Fanaroff-Riley class II (FRII) radio galaxies, matched with the sample of known X-shaped radio sources in size, morphological properties and redshift, using new Giant Metrewave Radio Telescope (GMRT) data and archival data from the Very Large Array (VLA).
D. Lal, M. J. Hardcastle, Ralph Kraft
openalex   +4 more sources

Relationship between X-shaped radio sources and double-double radio galaxies [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2006
AbstractBoth the X-shaped radio galaxies and double-double radio galaxies (DDRGs) are suggested in the literature to be due to the binary-accretion disk interaction or to the coalescence of SMBBHs. These models suggest some relationship between the two types of radio sources. In this paper, we collected data from literatures for two samples of X-shaped
Xian Chen, F. K. Liu
openalex   +3 more sources

The X-shaped Radio Galaxy J0725+5835 is Associated with an AGN Pair [PDF]

open access: goldThe Astrophysical Journal, 2022
Abstract X-shaped radio galaxies (XRGs) are those that exhibit two pairs of unaligned radio lobes (main radio lobes and wings). One of the promising models for the peculiar morphology is jet reorientation. To clarify this, we conducted a 5 GHz observation with the European VLBI Network (EVN) of XRG J0725+5835, which resembles the ...
Xiaolong Yang   +8 more
openalex   +3 more sources

Discovery of X-shaped morphology of the giant radio galaxy 0503-286 [PDF]

open access: hybridAstronomy & Astrophysics, 2022
The high surface-brightness sensitivity of the galactic and extragalactic all-sky mwa survey (GLEAM) image of the giant radio galaxy (GRG) 0503-28 at 70–230 MHz has revealed an inversion-symmetric bending of its two lobes, while maintaining a ∼200 kpc wide strip-like radio emission gap between their bent portions.
Pratik Dabhade, Gopal Krishna
openalex   +5 more sources

Starbursts and black hole masses in X-shaped radio galaxies: Signatures of a merger event? [PDF]

open access: bronzeAstronomy & Astrophysics, 2012
9 pages, 10 figures, accepted for publication in Astronomy & ...
Mar Mezcua   +3 more
  +8 more sources

X-shaped radio galaxies: probing jet evolution, ambient medium dynamics, and their intricate interconnection [PDF]

open access: goldFrontiers in Astronomy and Space Sciences
This review explores the field of X-shaped radio galaxies (XRGs), a distinctive subset of winged radio sources that are identified by two pairs of jetted lobes which aligned by a significant angle, resulting in an inversion-symmetric structure. These lobes, encompassing active (primary) and passive (secondary) phases, exhibit a diverse range of ...
Gourab Giri   +4 more
  +8 more sources

Deciphering the Morphological Origins of X-shaped Radio Galaxies: Numerical Modeling of Backflow versus Jet Reorientation [PDF]

open access: goldThe Astrophysical Journal Supplement Series, 2023
Abstract X-shaped radio galaxies (XRGs) develop when certain extragalactic jets deviate from their propagation path. An asymmetric ambient medium (backflow model) or complex active galactic nucleus activity (jet-reorientation model) enforcing the jet direction to deviate may cause these structures.
Gourab Giri   +2 more
openalex   +4 more sources

A VLBA-uGMRT search for candidate binary black holes: Study of six X-shaped radio galaxies with double-peaked emission lines [PDF]

open access: goldMonthly Notices of the Royal Astronomical Society
ABSTRACT Identifying methods to discover dual active galactic nucleus (AGN) has proven to be challenging. Several indirect tracers have been explored in the literature, including X/S-shaped radio morphologies and double-peaked (DP) emission lines in the optical spectra.
Biny Sebastian   +8 more
  +6 more sources

A radio-detected type Ia supernova with helium-rich circumstellar material. [PDF]

open access: yesNature, 2023
Kool EC   +36 more
europepmc   +1 more source

Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind. [PDF]

open access: yesNat Commun, 2023
Mou G   +8 more
europepmc   +1 more source

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