activity
20152022
most citedA tidal encounter caught in the act: modelling a star-disc fly-by in the young RW Aurigae system

91 citations · 518 across the 20 of their papers we have counts for

collaborators

26 papers

astro-ph.EP202220 cited

[OI] 6300Å emission as a probe of external photoevaporation of protoplanetary discs

Giulia Ballabio, Thomas J. Haworth, W. J. Henney

We study the utility of the [OI] 6300 forbidden line for identifying and interpreting externally driven photoevaporative winds in different environments and a…

astro-ph.GA202217 cited

Deep diving off the `Cosmic Cliffs': previously hidden outflows in NGC 3324 revealed by JWST

Megan Reiter, Jon A. Morse, Nathan Smith +3

We present a detailed analysis of the protostellar outflow activity in the massive star-forming region NGC 3324, as revealed by new Early Release Observations (ERO) from the James…

astro-ph.EP202245 cited

The evolution of protoplanetary discs in star formation and feedback simulations

Lin Qiao, Thomas J. Haworth, Andrew D. Sellek +1

We couple star cluster formation and feedback simulations of a Carina-like star forming region with 1D disc evolutionary models to study the impact of external photoevaporation on…

astro-ph.EP20229 cited

An APEX search for carbon emission from NGC 1977 proplyds

Thomas J. Haworth, Jinyoung S. Kim, Lin Qiao +8

We used the Atacama Pathfinder Experiment (APEX) telescope to search for CI 1-0 (492.16GHz) emission towards 8 proplyds in NGC 1977, which is an FUV radiation environment two order…

astro-ph.EP202218 cited

Determining dispersal mechanisms of protoplanetary disks using accretion and wind mass loss rates

Yasuhiro Hasegawa, Thomas J. Haworth, Keri Hoadley +6

Understanding the origin of accretion and dispersal of protoplanetary disks is fundamental for investigating planet formation. Recent numerical simulations show that launching wind…

astro-ph.GA202116 cited

PION: Simulating bow shocks and circumstellar nebulae

Jonathan Mackey, Samuel Green, Maria Moutzouri +4

Expanding nebulae are produced by mass loss from stars, especially during late stages of evolution. Multi-dimensional simulation of these nebulae requires high resolution near the…