Results 1 to 10 of about 703 (116)

An Old Fogey’s History of Radio Jets [PDF]

open access: yesGalaxies, 2017
This paper describes a personal view of the discovery of radio jets in celestial radio sources. The existence of narrow, collimated optical features in distant objects has been known about since the early 20th century; however, the advent of radio ...
Ralph Spencer
doaj   +5 more sources

Radio jet precession in M 81* [PDF]

open access: yesAstronomy & Astrophysics, 2023
We report four novel position angle measurements of the core region M 81* at 5 GHz and 8 GHz, which confirm the presence of sinusoidal jet precession in the M 81 jet region, as suggested by Martí-Vidal et al. (2011, A&A, 533, A111). The model makes three testable predictions regarding the evolution of the jet precession, which we test in our data ...
S. D. von Fellenberg   +7 more
openaire   +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

Wide-Angle-Tail (WAT) Radio Sources

open access: yesGalaxies, 2023
We review the properties of Wide-Angle-Tail (WAT) radio sources. The WAT radio sources are powerful, bent radio sources typically associated with the dominant galaxy in a cluster or group.
Christopher P. O’Dea, Stefi A. Baum
doaj   +1 more source

Radio Emission of Nearby Early-type Galaxies in the Low and Very Low Radio Luminosity Range

open access: yesThe Astrophysical Journal, 2023
We analyze radio continuum emission of early-type galaxies with dynamical measurements of central supermassive black hole (SMBH) masses and well-characterized large-scale environments, but regardless of the exact level of the nuclear activity.
Anna Wójtowicz   +4 more
doaj   +1 more source

Optical Observations of Radio Jets [PDF]

open access: yesHighlights of Astronomy, 1980
Over the past several years a considerable body of evidence has accumulated, suggesting that extended radio sources are powered quasi-continuously from the nuclei of their parent galaxies. This view is supported by the recent discovery that several radio galaxies have narrow radio jets which connect their active nuclei with the large radio lobes and ...
Butcher, H.R.   +2 more
openaire   +3 more sources

What Drives the Ionized Gas Outflows in Radio-Quiet AGN?

open access: yesGalaxies, 2023
We review the mechanisms driving the ionized gas outflows in radio-quiet (RQ) AGN. Although it constitutes ∼90% of the AGN population, what drives these outflows in these AGNs remains an open question. High-resolution imaging and integral field unit (IFU)
Mainak Singha   +2 more
doaj   +1 more source

Offsets between X-Ray and Radio Components in X-Ray Jets: The AtlasX

open access: yesThe Astrophysical Journal Supplement Series, 2023
The X-ray emission mechanism of powerful extragalactic jets—which has important implications for their environmental impacts—is poorly understood. The X-ray/radio positional offsets in the individual features of jets provide important clues.
Karthik Reddy   +4 more
doaj   +1 more source

Narrow-Line Seyfert 1 Galaxies With Absorbed Jets–Insights From Radio Spectral Index Maps

open access: yesFrontiers in Astronomy and Space Sciences, 2021
Narrow-line Seyfert 1 (NLS1) galaxies are active galactic nuclei (AGN) believed to be in the early stages of their evolution. A fraction of them have been found to host relativistic jets.
Emilia Järvelä    +3 more
doaj   +1 more source

The Radio Jet in 3C418 [PDF]

open access: yesSymposium - International Astronomical Union, 1984
Models are here presented interpreting the arcsecond radio structure found in the quasar 3C418 as a precessing jet. No simple solution exists and it has been found necessary to complicate the model geometry by allowing the precession cone-angle to increase with time.
T.W.B. Muxlow, M. Jullian, R. Linfield
openaire   +1 more source

Home - About - Disclaimer - Privacy