activity
20152023
most citedThe impact of pre-supernova feedback and its dependence on environment

55 citations · 183 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2023

Star cluster formation and feedback in different environments of a Milky Way-like galaxy

Ahmad A. Ali, Clare L. Dobbs, Thomas J. R. Bending +2

It remains unclear how galactic environment affects star formation and stellar cluster properties. This is difficult to address in Milky Way-mass galaxy simulations because of limi…

astro-ph.GA202218 cited

Stellar winds and photoionization in a spiral arm

Ahmad A. Ali, Thomas J. R. Bending, Clare L. Dobbs

The role of different stellar feedback mechanisms in giant molecular clouds is not well understood. This is especially true for regions with many interacting clouds as would be fou…

astro-ph.GA202155 cited

The impact of pre-supernova feedback and its dependence on environment

Anna F. Mcleod, Ahmad A. Ali, Mélanie Chevance +8

Integral field units enable resolved studies of a large number of star-forming regions across entire nearby galaxies, providing insight on the conversion of gas into stars and the…

astro-ph.GA202132 cited

The growth of H II regions around massive stars: the role of metallicity and dust

Ahmad A. Ali

Gas metallicity and the related dust-to-gas ratio can influence the growth of HII regions via metal line cooling and UV absorption. We model these effects in sta…

astro-ph.GA20201 cited

Shape Analysis of HII Regions -- II. Synthetic Observations

Justyn Campbell-White, Ahmad A. Ali, Dirk Froebrich +1

The statistical shape analysis method developed for probing the link between physical parameters and morphologies of Galactic HII regions is applied here to a set of synthetic obse…

astro-ph.GA201932 cited

Massive star feedback in clusters: variation of the FUV interstellar radiation field in time and space

Ahmad A. Ali, Tim J. Harries

We investigate radiative feedback from a 34 M star in a M turbulent cloud using three-dimensional radiation-hydrodynamics (RHD) models. We use Monte Carlo ra…