Saved in:
| Main Author: | |
|---|---|
| Format: | Preprint |
| Published: |
2026
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2603.28585 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Table of Contents:
- Polarization provides additional diagnostic opportunities for probing the structured environments of massive stars as well as the illumination of those environments by stars that are not spherical. After a brief overview of polarization considerations relevant to hot massive stars, selected applications are presented. Examples related to dense Wolf-Rayet winds are chosen: clumpy wind flow, co-rotating interaction regions, and colliding wind interactions. Brief remarks are given about the prospects for opening a new window on massive star studies using UV spectropolarimetry with the {\em Polstar} mission concept.