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20152021
most citedAsymmetric jet production in the Active Galactic Nucleus of NGC1052

44 citations · 134 across the 9 of their papers we have counts for

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7 papers · 1 filter

astro-ph.GA202115 cited

Apertif view of the OH Megamaser IRAS 10597+5926: OH 18 cm satellite lines in wide-area HI surveys

Kelley M. Hess, H. Roberts, H. Dénes +26

We present the serendipitous detection of the two main OH maser lines at 1667 and 1665 MHz associated with IRAS 10597+5926 at z = 0.19612 in the untargeted Apertif Wide-area Extrag…

astro-ph.GA2020

The parsec-scale HI outflows in powerful radio galaxies

R. Schulz, R. Morganti, K. Nyland +3

Massive outflows of neutral atomic hydrogen (HI) have been observed in absorption in a number of radio galaxies and are considered a signature of AGN feedback. These outflows on kp…

astro-ph.GA20209 cited

Extreme intra-hour variability of the radio source J1402+5347 discovered with Apertif

T. A. Oosterloo, H. K. Vedantham, A. M. Kutkin +27

The propagation of radio waves from distant compact radio sources through turbulent interstellar plasma in our Galaxy causes these sources to twinkle, a phenomenon called interstel…

astro-ph.GA2019

Feedback from low-luminosity radio galaxies: B2 0258+35

Suma Murthy, Raffaella Morganti, Tom Oosterloo +6

Low-luminosity radio-loud active galactic nuclei (AGN) are of importance in studies concerning feedback from radio AGN since a dominant fraction of AGN belong to this class. We rep…

astro-ph.GA201944 cited

Asymmetric jet production in the Active Galactic Nucleus of NGC1052

A. -K. Baczko, R. Schulz, M. Kadler +4

Context: Few Active Galactic Nuclei (AGN) reveal a double sided jet system. However, these are crucial to understand basic physical properties of extragalactic jets. Aims: We addre…

astro-ph.GA20191 cited

The parsec-scale structure of jet-driven HI outflows in radio galaxies

Raffaella Morganti, Robert Schulz, Kristina Nyland +4

Radio jets can play multiple roles in the feedback loop by regulating the accretion of the gas, by enhancing gas turbulence, and by driving gas outflows. Numerical simulations are…