Back to Volume
Paper: The Quasi-WR Star HD 45166 Revisited
Volume: 519, Radiative Signatures from the Cosmos
Page: 197
Authors: Dolevzalová, B.; Kubátová, B.; Kubát, J.; Hamann, W.
Abstract: 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.
Back to Volume