Michael Boylan-Kolchin

7 ta ish

The University of Texas at Austin

1. FIRE-2 simulations: physics versus numerics in galaxy formation

   Philip F. Hopkins, Andrew Wetzel, Dušan Kereš +25

   Maqola20185 iqtibos

   ABIABI:AkademIndex/2026.other.467823

2. Small-Scale Challenges to the <b><i>Λ</i></b>CDM Paradigm

   James S. Bullock, Michael Boylan-Kolchin

   Maqola20173 iqtibos

   ABIABI:AkademIndex/2026.other.790027

3. The Milky Way’s bright satellites as an apparent failure of ΛCDM

   Michael Boylan-Kolchin, James S. Bullock, Manoj Kaplinghat

   MaqolaOAOchiq kirish20122 iqtibos

   ABIABI:AkademIndex/2026.other.011249

4. From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology

   Qi Guo, Simon D. M. White, Michael Boylan-Kolchin +6

   Maqola20112 iqtibos

   ABIABI:AkademIndex/2026.other.370000

5. Where are the most ancient stars in the Milky Way?

   Kareem El-Badry, Joss Bland‐Hawthorn, Andrew Wetzel +7

   Maqola20182 iqtibos

   ABIABI:AkademIndex/2026.other.797786

6. Stress testing ΛCDM with high-redshift galaxy candidates

   Michael Boylan-Kolchin

   Maqola20231 iqtibos

   ABIABI:AkademIndex/2026.other.467779

7. COSMOS-Web: Intrinsically Luminous z ≳ 10 Galaxy Candidates Test Early Stellar Mass Assembly

   Caitlin M. Casey, Hollis B. Akins, Marko Shuntov +39

   Maqola20241 iqtibos

   ABIABI:AkademIndex/2026.other.467783