Tag Archives: 21cm

18 May 2022

  • (abs, pdf) Chiaki & Wise, Triggered Population III star formation: the effect of H$_2$ self-shielding
  • (abs, pdf) Schatz et al., Horizons: Nuclear Astrophysics in the 2020s and Beyond
  • (abs, pdf) Piras et al., Fast and realistic large-scale structure from machine-learning-augmented random field simulations
  • (abs, pdf) Ricotti et al., Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
  • (abs, pdf) Zier & Springel, Simulating cold shear flows on a moving mesh
  • (abs, pdf) Seitova & Pober, The Optical Depth of Foregrounds for the Highest Redshift 21 cm Signals

22 Mar 2022

  • (abs, pdf) Li et al., On the Connection between Supermassive Black Hole and Galaxy Growth in the Reionization Epoch
  • (abs, pdf) Kaur et al., The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries
  • (abs, pdf) Rodriguez-Gomez et al., Galactic angular momentum in the IllustrisTNG simulation — I. Connection to morphology, halo spin, and black hole mass
  • (abs, pdf) Munive-Villa et al., Solving the Schrodinger Poisson System using the coordinate Adaptive Moving Mesh method

20 Jan 2022

  • (abs, pdf) Weller et al., Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
  • (abs, pdf) Fichtner et al., Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
  • (abs, pdf) Mirocha et al., A galaxy-free phenomenological model for the 21-cm power spectrum during reionization
  • (abs, pdf) Wurster et al., On the origin of magnetic fields in stars II: The effect of numerical resolution
  • (abs, pdf) Yoshioka et al., CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC
  • (abs, pdf) Armitage, Lecture notes on accretion disk physics
  • (abs, pdf) Hunter et al., Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies