First author (6 total)
- Semenov, Kravtsov, Caprioli 2020 | arXiv:2012.01427
Cosmic Ray Diffusion Suppression in Star-Forming Regions Inhibits Clump Formation in Gas-Rich Galaxies - Semenov, Kravtsov, Gnedin 2019 | ApJ 870, 79 | arXiv:1809.07328
What Sets the Slope of the Molecular Kennicutt–Schmidt Relation? - Semenov, Kravtsov, Gnedin 2018 | ApJ 861, 4 | arXiv:1803.00007
How Galaxies Form Stars: the Connection between Local and Global Star Formation in Galaxy Simulations - Semenov, Kravtsov, Gnedin 2017 | ApJ 845, 133 | arXiv:1704.04239
The Physical Origin of Long Gas Depletion Times in Galaxies - Semenov, Kravtsov, Gnedin 2016 | ApJ 826, 200 | arXiv:1512.03101
Nonuniversal Star Formation Efficiency in Turbulent ISM - Semenov 2013 | Astronomy Reports 57, 485
Statistical Analysis of the Large-Scale Structure of the Universe Using Observational Data and Numerical Modeling
In collaboration (3 total)
- Gnedin, Semenov, Kravtsov 2018 | J. Comput. Phys. 359, 93 | arXiv:1801.03108
Enforcing the Courant–Friedrichs–Lewy Condition in Explicitly Conservative Local Time Stepping Schemes - Li, Gnedin, Gnedin, Meng, Semenov, Kravtsov 2017 | ApJ 834, 69 | arXiv:1608.03244
Star Cluster Formation in Cosmological Simulations. I. Properties of Young Clusters - Kim et al. (AGORA Collaboration) 2016 | ApJ 833, 202 | arXiv:1610.03066
The AGORA High-resolution Galaxy Simulations Comparison Project. II. Isolated Disk Test