104 citations · 178 across the 7 of their papers we have counts for
7 papers
The long-term effects of gas removal from hydrodynamic simulations of star formation
Aleksandra Calovic, Katerina S. Klos, Robert B. Hudson +2
The removal of gas left over from star formation has long been thought to dominate the dynamical evolution, and dissolution of star-forming regions. Feedback from massive stars fro…
Signatures of mass segregation from competitive accretion and monolithic collapse
Richard J. Parker, Emily J. Pinson, Hayley L. Alcock +1
The two main competing theories proposed to explain the formation of massive (M) stars -- competitive accretion and monolithic core collapse -- make different observab…
Isolating signatures of major cloud-cloud collisions II: The lifetimes of broad bridge features
T. J. Haworth, K. Shima, E. J. Tasker +5
We investigate the longevity of broad bridge features in position-velocity diagrams that appear as a result of cloud-cloud collisions. Broad bridges will have a finite lifetime due…
Photoionising feedback and the star formation rates in galaxies
J. M. MacLachlan, I. A. Bonnell, K. Wood +1
Aims. We investigate the effects of ionising photons on accretion and stellar mass growth in a young star forming region, using a Monte Carlo radiation transfer code coupled to a s…
Old pre-main-sequence Stars: Disc reformation by Bondi-Hoyle accretion
P. Scicluna, G. Rosotti, J. E. Dale +1
Young stars show evidence of accretion discs which evolve quickly and disperse with an e-folding time of 3Myr. This is in striking contrast with recent observations that sug…
Imprints of feedback in young gasless clusters?
Richard J. Parker, James E. Dale
We present the results of N-body simulations in which we take the masses, positions and velocities of sink particles from five pairs of hydrodynamical simulations of star formation…
The Impact of Stellar Collisions in the Galactic Center
M. B. Davies, R. P. Church, D. Malmberg +3
We consider whether stellar collisions can explain the observed depletion of red giants in the Galactic center. We model the stellar population with two different IMFs: 1) the Mill…