The Quasi-WR Star HD 45166 Revisited
Dolezalova, Barbora; Kubatova, Brankica; Kubat, Jiri; Hamann, Wolf-Rainer
We studied the wind of the quasi Wolf-Rayet (qWR) star HD 45166. As a first step we modeled the observed UV spectra of this star by means of the state-of-the-art Potsdam Wolf-Rayet (PoWR) atmosphere code. We inferred the wind parameters and compared them with previous findings.