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20112023
most citedRelativistic jet feedback III: feedback on gas disks

258 citations · 2k across the 48 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.GA2021★ 47 cited

Impact of relativistic jets on the star formation rate: a turbulence-regulated framework

Ankush Mandal, Dipanjan Mukherjee, Christoph Federrath +4

We apply a turbulence-regulated model of star formation to calculate the star formation rate (SFR) of dense star-forming clouds in simulations of jet-ISM interactions. The method i…

astro-ph.GA2021★ 18 cited

Resolved simulations of jet-ISM interaction: Implications for gas dynamics and star formation

Dipanjan Mukherjee, Geoffrey V. Bicknell, Alexander Y. Wagner

Relativistic jets can interact with the ambient gas distribution of the host galaxy, before breaking out to larger scales. In the past decade several studies have simulated jet-dri…

astro-ph.HE2021★ 19 cited

Tracing the Milky Way's Vestigial Nuclear Jet

Gerald Cecil, Alexander Y. Wagner, Joss Bland-Hawthorn +2

MeerKAT radio continuum and XMM-Newton X-ray images have recently revealed a spectacular bipolar channel at the Galactic Center that spans several degrees (0.5 kpc). An inter…

astro-ph.HE2021★ 23 cited

Morphology of radio relics II: Properties of polarised emission

P. Domínguez-Fernández, M. Brüggen, F. Vazza +7

Radio relics are diffuse radio sources in galaxy clusters that are associated with merger shock waves. Detailed observations of radio relics in total intensity and in polarisation…

astro-ph.GA2021★ 16 cited

AGN Jets and Winds in Polarised Light: The Case of Mrk 231

Silpa S., P. Kharb, C. P. O' Dea +4

We present the results of a multi-frequency, multi-scale radio polarimetric study with the Very Large Array (VLA) of the Seyfert 1 galaxy and BALQSO, Mrk 231. We detect complex tot…

astro-ph.HE2021★ 49 cited

Simulating the dynamics and synchrotron emission from relativistic jets II. Evolution of non-thermal electrons

Dipanjan Mukherjee, Gianluigi Bodo, Paola Rossi +2

We have simulated the evolution of non-thermal cosmic ray electrons (CREs) in 3D relativistic magneto hydrodynamic (MHD) jets evolved up to a height of 9 kpc. The CREs have been ev…