The Quasi-WR Star HD 45166 Revisited

Investor logo

Warning

This publication doesn't include Faculty of Arts. It includes Faculty of Science. Official publication website can be found on muni.cz.
Authors

DOLEŽALOVÁ Barbora KUBÁTOVÁ Brankica KUBÁT Jiří HAMANN Wolf-Rainer

Year of publication 2019
Type Article in Proceedings
Conference Radiative Signatures from the Cosmos
MU Faculty or unit

Faculty of Science

Citation
Web http://www.aspbooks.org/a/volumes/table_of_contents/?book_id=590
Keywords HD 45166; stellar wind; quasi Wolf-Rayet star;PoWR
Description 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.
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.