Results 21 to 30 of about 1,237,003 (361)

Radio jets from AGNs in dwarf galaxies in the COSMOS survey: mechanical feedback out to redshift ∼3.4 [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
Dwarf galaxies are thought to host the remnants of the early Universe seed black holes (BHs) and to be dominated by supernova feedback. However, recent studies suggest that BH feedback could also strongly impact their growth. We report the discovery of
M. Mezcua, H. Suh, F. Civano
semanticscholar   +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

Radio jets and gamma-ray emission in radio-silent narrow-line Seyfert 1 galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2018
We have detected six narrow-line Seyfert 1 (NLS1) galaxies at 37 GHz that were previously classified as radio silent and two that were classified as radio quiet.
A. Lähteenmäki   +6 more
semanticscholar   +1 more source

Fast-spinning Black Holes Inferred from Symmetrically Limb-brightened Radio Jets [PDF]

open access: yesAstrophysical Journal, 2018
This paper theoretically investigates the relations between the structure of relativistic jets and produced synchrotron images, by using a steady, axisymmetric force-free jet model.
Kazuya Takahashi   +4 more
semanticscholar   +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

Finding Rare Quasars: VLA Snapshot Continuum Survey of FRI Quasar Candidates Selected from the LOFAR Two-Metre Sky Survey (LoTSS)

open access: yesGalaxies, 2021
The radiative and jet power in active galactic nuclei is generated by accretion of material on to supermassive galactic-centre black holes. For quasars, where the radiative power is by definition very high, objects with high radio luminosities form 10 ...
Gülay Gürkan   +5 more
doaj   +1 more source

The many lives of active galactic nuclei–II: The formation and evolution of radio jets and their impact on galaxy evolution [PDF]

open access: yes, 2017
We describe new efforts to model radio active galactic nuclei (AGN) in a cosmological context using the Semi-Analytic Galaxy Evolution (SAGE) semi-analytic galaxy model.
Mojtaba Raouf   +4 more
semanticscholar   +1 more source

Gas kinematics in powerful radio galaxies at z ~ 2: Energy supply from star formation, AGN, and radio jets [PDF]

open access: yes, 2016
We compare the kinetic energy and momentum injection rates from intense star formation, bolometric AGN radiation, and radio jets with the kinetic energy and momentum observed in the warm ionized gas in 24 powerful radio galaxies at z~2.
N. Nesvadba   +5 more
semanticscholar   +1 more source

The Radio Jet of 3C273 [PDF]

open access: yesSymposium - International Astronomical Union, 1982
Most radio sources are two-sided, like Cygnus A. A minority, however, are one-sided, and the first-known and brightest example is 3C273 (see Fig. 1), a high-luminosity QSO, showing ‘super-luminal’ proper motions in the core. The explanation of such one-sided sources may follow one of two lines (and it seems that both schools of thought are represented ...
openaire   +2 more sources

A candidate dual AGN in a double-peaked emission-line galaxy with precessing radio jets [PDF]

open access: yes, 2016
We present high resolution radio continuum observations with the Karl G. Jansky Very Large Array at 6, 8.5, 11.5 and 15 GHz of the double-peaked emission-line galaxy 2MASXJ12032061+1319316.
K. Rubinur   +5 more
semanticscholar   +1 more source

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