2022 (v1)
Journal article
Context. Achernar, the closest and brightest classical Be star, presents rotational flattening, gravity darkening, occasional emission lines due to a gaseous disk, and an extended polar wind. It is also a member of a close binary system with an early A-type dwarf companion. Aims: We aim to determine the orbital parameters of the Achernar...
Uploaded on: December 3, 2022