activity
20032026
most citedExtended radio emission in MOJAVE Blazars: Challenges to Unification

151 citations · 3.7k across the 163 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2019

Understanding the Origin of Radio Outflows in Seyfert Galaxies using Radio Polarimetry

Biny Sebastian, P. Kharb, C. P. O' Dea +3

The role of starburst winds versus active galactic nuclei (AGN) jets/winds in the formation of the kiloparsec scale radio emission seen in Seyferts is not yet well understood. In o…

astro-ph.GA2019★ 19 cited

The Discovery of Secondary Lobes in the Seyfert Galaxy NGC 2639

Biny Sebastian, P. Kharb, C. P. O`Dea +2

We report the discovery of a secondary pair of radio lobes in the Seyfert galaxy NGC 2639 with polarization-sensitive observations with the Karl G. Jansky Very Large Array (VLA). T…

astro-ph.GA2019★ 23 cited

The filamentary radio lobes of the Seyfert-Starburst composite galaxy NGC3079

Biny Sebastian, Preeti Kharb, C. P. O Dea +2

We present results from multi-frequency polarization-sensitive Very Large Array observations of the Seyfert-starburst composite galaxy NGC3079. Our sensitive radio observations rev…

astro-ph.GA2019★ 9 cited

Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA

David R. A. Williams, Ian M. McHardy, Ranieri D. Baldi +13

We present high-sensitivity 1.51 GHz e-MERLIN radio images of the nearby galaxy NGC 6217. We resolve the compact radio source at the centre of NGC 6217 for the first time, finding…

astro-ph.GA2019★ 10 cited

Gemini IFU, VLA, and HST observation of the OH Megamaser Galaxy IRAS17526+3253

Dinalva A. Sales, A. Robinson, R. A. Riffel +7

We present a multiwavelength study of the OH megamaser galaxy (OHMG) IRAS17526+3253, based on new Gemini Multi-Object Spectrograph Integral Field Unit (GMOS/IFU) observations, Hubb…

astro-ph.GA2019★ 47 cited

Searching for Dual AGN in Galaxies with Double-Peaked Emission Line Spectra using Radio Observations

K. Rubinur, M. Das, P. Kharb

Supermassive black hole (SMBH) binaries form due to galaxy mergers and minor accretion events. When the SMBHs are accreting, they form dual or binary AGN and can give rise to doubl…