Results 31 to 40 of about 9,758 (163)

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

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

A Unified Framework for X-shaped Radio Galaxies

open access: hybridThe Astrophysical Journal, 2020
Abstract We propose a radically different picture for X-shaped radio galaxies compared with existing models as transition objects between cold-mode accreting, low-spinning retrograde black holes and low-spinning prograde black holes. This model explains their smaller average black hole masses; their general aversion for cluster compared ...
David Garofalo   +5 more
openalex   +3 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: greenMonthly 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

Discovery of Giant Bubbles in the Hot Gaseous Halo of the Massive Disk Galaxy NGC 6286

open access: yesThe Astrophysical Journal
Based on archival Chandra X-ray observation, optical integral-field spectroscopic data, and radio interferometric data, we report the discovery of a pair of giant bubbles (with a projected radius ∼5 kpc) of ionized gas emerging from a highly inclined ...
Lin He   +5 more
doaj   +2 more sources

Jet Interaction with Galaxy Cluster Mergers

open access: yesThe Astrophysical Journal
Active galactic nucleus (AGN) bubbles in cool-core galaxy clusters are believed to facilitate the transport of cosmic-ray electrons (CRe) throughout the cluster.
P. Domínguez-Fernández   +6 more
doaj   +2 more sources

Massive black hole binaries as sources of low-frequency gravitational waves and X-shaped radio galaxies [PDF]

open access: goldMonthly Notices of the Royal Astronomical Society
ABSTRACT We present the study of multimessenger signatures of massive black hole (MBH) binaries residing in the centres of galaxy merger remnants. In particular, we first focus on the gravitational wave background (GWB) produced by an ensemble of MBH binary inspirals in the frequency range probed by the Pulsar Timing Array (PTA ...
M. Curyło, T. Bulik
openalex   +3 more sources

Evidence for In - Situ Acceleration of Relativistic Particles in the Wings of X-shaped Radio Galaxies

open access: goldThe Astrophysical Journal
Abstract We report evidence for in - situ acceleration/reacceleration of relativistic particles in 11 radio wings out of a total of 68 wings sufficiently well-resolved for spectral mapping, which belong to our sample of 40 X-shaped ...
Dusmanta Patra   +2 more
  +5 more sources

Origin of the double-peaked narrow emission-lines in the optical spectra of X-shaped Radio Galaxies [PDF]

open access: green
We investigate the X-shaped radio galaxies (XRGs) with optical double-peaked narrow emission (DPNEL) as potential hosts of dual or binary supermassive black holes (SMBHs). Using a sample of 187 XRGs selected from SDSS and DESI optical spectroscopic surveys, we check the AGN nature of both emission components using the BPT diagnostics of multiple ...
P. Ghosh   +13 more
openalex   +3 more sources

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