3 papers
astro-ph.GA2026
TRINITY: A coupled model of winds, radiation, and photoionised gas in molecular clouds. I. Methods and validation
Jia Wei Teh, Ralf S. Klessen, Simon C. O. Glover +1
Multi-wavelength surveys place cloud dispersal at 1-5 Myr after massive stars emerge, before the first supernovae. Whether a cloud disperses, re-collapses, or leaks Lyman-continuum…
astro-ph.GA2026
Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons
Fabian Scheuermann, Kathryn Kreckel, Jia Wei Teh +27
Newly formed stars have a profound impact on their environment by depositing energy and momentum into the surrounding gas. However, only a fraction of the stellar feedback is retai…
astro-ph.GA2025
Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +11
The mode of star formation that results in the formation of globular clusters and young massive clusters is difficult to constrain through observations. We present models of massiv…