TY  CONF
TI  MHD-Modeling of the molecular filament evolution with numerical FLASH code
KW  ISM: clouds
KW  evolution
KW  magnetic fields; magnetohydrodynamics (MHD); methods: numerical
JO  Modern astronomy: from the Early Universe to exoplanets and black holes
AU  Sultanov, I..
AU  Khaibrakhmanov, S..
PY  2024
PB  Special Astrophysical Observatory of the Russian Academy of Sciences