The simulation of molecular clouds formation in the Milky Way
Sergey Khoperskov(Centre National de la Recherche Scientifique), А. В. Хоперсков(Volgograd State University), А. М. Соболев(Ural Federal University), E. O. Vasiliev(P.N. Lebedev Physical Institute of the Russian Academy of Sciences)
Cited by 44
Related Papers
The Milky Way has no in-situ halo other than the heated thick disc
|Astronomy and Astrophysics|2019|211
Review of scientific topics for the Millimetron space observatory
|Physics-Uspekhi|2014|138
Bar quenching in gas-rich galaxies
|Astronomy and Astrophysics|2017|110
StarHorse results for spectroscopic surveys and <i>Gaia</i> DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars
|Astronomy and Astrophysics|2023|99
The disc origin of the Milky Way bulge
|Astronomy and Astrophysics|2018|86