TY  CONF
TI  Wolf–Rayet stars mass-loss rates determined from spectroscopic measurements of the orbital evolution for close WR+OB binary systems
KW  stars: Wolf–Rayet
KW  mass-loss
KW  winds
KW  outflows
KW  binaries: spectroscopic
JO  Modern astronomy: from the Early Universe to exoplanets and black holes
AU  Shaposhnikov, I..
PY  2024
PB  Special Astrophysical Observatory of the Russian Academy of Sciences