Tag Archives: MW

31 Oct 2019

  • (abs, pdf) Lofthouse et al., MUSE Analysis of Gas around Galaxies (MAGG) — I: Survey design and the environment of a near pristine gas cloud at z~3.5
  • (abs, pdf) Mandal et al., Molecular cloud formation by compression of magnetized turbulent gas subjected to radiative cooling
  • (abs, pdf) Di Matteo et al., Reviving old controversies: is the early Galaxy flat or round? Investigations into the early phases of the Milky Way formation through stellar kinematics and chemical abundances

09 Aug 2019

  • (abs, pdf) Deason et al., The total stellar halo mass of the Milky Way
  • (abs, pdf) Hilker et al., Galactic globular clusters: a new catalog of masses, structural parameters, velocity dispersion profiles, proper motions and space orbits
  • (abs, pdf) Bhowmick et al., Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
  • (abs, pdf) Regan et al., The Emergence of the First Star-free Atomic Cooling Haloes in the Universe

18 Apr 2019

  • (abs, pdf) Muñoz, A Standard Ruler at Cosmic Dawn
  • (abs, pdf) Sameie et al., Self-Interacting Dark Matter Subhalos in the Milky Way's Tides
  • (abs, pdf) Muñoz, Velocity-induced Acoustic Oscillations at Cosmic Dawn
  • (abs, pdf) He et al., Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies
  • (abs, pdf) Vanzella et al., Ionising the Intergalactic Medium by Star Clusters ? The first empirical evidence
  • (abs, pdf) Lorente et al., Moving Towards Greater Equity, Diversity, and Inclusion in Astronomy

09 Apr 2019

  • (abs, pdf) Myeong et al., Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
  • (abs, pdf) Neyrinck et al., Halo Spin from Primordial Inner Motions
  • (abs, pdf) Ezzeddine et al., Evidence for an aspherical Population III supernova explosion inferred from the hyper metal-poor star HE1327-2326
  • (abs, pdf) Doussot et al., Improved supervised learning methods for EoR parameters reconstruction
  • (abs, pdf) Viganò & Palenzuela, Fitting of extended sub-grid scale models in compressible turbulent MHD