Innovative measurements of stellar mass loss
Abstract
Analysis of archival XMM-Newton data yields measurements of stellar wind emission from three star systems, illustrating a direct method to determine the mass-loss rates of late-type main-sequence stars.
- Publication:
-
Nature Astronomy
- Pub Date:
- May 2024
- DOI:
- 10.1038/s41550-024-02227-6
- Bibcode:
- 2024NatAs...8..551W