activity
20172022
most citedFollow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

212 citations · 236 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202224 cited

The SAMI Galaxy Survey: the difference between ionised gas and stellar velocity dispersions

Sree Oh, Matthew Colless, Francesco D'Eugenio +16

We investigate the mean locally-measured velocity dispersions of ionised gas () and stars () for 1090 galaxies with stellar masses $\log\,(M_*/M_{\odot}) \geq 9.5…

astro-ph.GA2021

Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with bright X-ray halo

N. P. H. Nesvadba, A. Y. Wagner, D. Mukherjee +6

It has long been suspected that powerful radio sources may lower the efficiency with which stars form from the molecular gas in their host galaxy, but so far, alternative mechanism…

astro-ph.GA2020

Unravelling the enigmatic ISM conditions in Minkowski's Object

Henry R. M. Zovaro, Robert Sharp, Nicole P. H. Nesvadba +7

Local examples of jet-induced star formation lend valuable insight into its significance in galaxy evolution and can provide important observational constraints for theoretical mod…

astro-ph.GA2019

Searching for signs of jet-driven negative feedback in the nearby radio galaxy UGC 05771

Henry R. M. Zovaro, Nicole P. H. Nesvadba, Robert Sharp +4

Hydrodynamical simulations predict that the jets of young radio sources can inhibit star formation in their host galaxies by injecting heat and turbulence into the interstellar med…

astro-ph.GA2018

Jets blowing bubbles in the young radio galaxy 4C 31.04

Henry R. M. Zovaro, Robert Sharp, Nicole P. H. Nesvadba +5

We report the discovery of shocked molecular and ionized gas resulting from jet-driven feedback in the compact radio galaxy 4C 31.04 using near-IR imaging spectroscopy. 4C 31.04 is…

astro-ph.HE2017212 cited

Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

I. Andreoni, K. Ackley, J. Cooke +122

The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era…