An impressionist view of V Hydrae. When MATISSE paints asymmetric giant blobs
Context. Asymptotic giant branch (AGB) stars enrich the interstellar medium through their mass loss. The mechanism(s) shaping the circumstellar environment of mass-losing stars is not clearly understood so far. Aims: Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this
Planquart, L. et al.
Fecha de publicación:
7
2024