机译:A MOST probable explanation of the pulsation of WR 123
Univ Vienna, Inst Astron, A-1180 Vienna, Austria;
Tohoku Univ, Inst Astron, Sendai, Miyagi 980, Japan;
ost.tau.ac.il;
stars : massive; stars : pulsations; stars : individual : WR123; WOLF-RAYET STARS; STRANGE MODES; NONRADIAL PULSATIONS; MASSIVE STARS; INSTABILITIES; PARAMETERS; ORIGIN;