Abstract
A search for variability in the extreme helium star LSS 3184 shows at least one frequency (period ~ 0.107 d; semi-amplitude ~ 0.01 mag in B) and the first harmonic. This agrees with the prediction by Saio that the star should pulsate, unless very metal-weak, due to the classical kappa mechanism and the iron opacity bump near 2 × 105 K.

This publication has 0 references indexed in Scilit: