Showing 1–20 of 20 results
/ Date/ Name
Jan 31, 2023Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022Feb 1, 2024The Energy and Dynamics of Trapped Radiative Feedback with Stellar WindsDec 1, 2014A Detailed Study of Feedback from a Massive StarJun 27, 2018On the Indeterministic Nature of Star Formation on the Cloud ScaleJun 13, 2019When H II Regions are Complicated: Considering Perturbations from Winds, Radiation Pressure, and Other EffectsMar 29, 2017Interpreting the Star Formation Efficiency of Molecular Clouds with Ionising FeedbackApr 15, 2012Satellite Survival in Highly Resolved Milky Way Class HalosJan 11, 2011How Does Feedback Affect Milky Way Satellite Formation?Sep 18, 2020The Geometry and Dynamical Role of Stellar Wind Bubbles in Photoionised HII RegionsNov 5, 2021Bottling the Champagne: Dynamics and Radiation Trapping of Wind-Driven Bubbles around Massive StarsJul 10, 2015Photoionisation Feedback in a Self-Gravitating, Magnetised, Turbulent CloudJul 19, 2016Feedback in Clouds II: UV Photoionisation and the first supernova in a massive cloudJan 16, 2020Simulating Star Clusters Across Cosmic Time: II. Escape Fraction of Ionizing Photons from Molecular CloudsFeb 4, 2022Influence of protostellar jets and HII regions on the formation and evolution of stellar clustersSep 4, 2018Impact of galactic shear and stellar feedback on star formationFeb 20, 2022Trapping of HII regions in Population III star formationFeb 22, 2022The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped windsApr 16, 2019Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and EfficienciesSep 14, 2022The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clustersOct 6, 2021A systematic study of the escape of LyC and Ly$α$ photons from star-forming, magnetized turbulent clouds