Interferometry of Massive Stars: Multiplicity, Magnetism, and Stellar Winds
Solar and Stellar Astrophysics
2025-12-02 v1 Instrumentation and Methods for Astrophysics
Abstract
After decades of efforts, optical long-baseline interferometry has become a mainstream observational technique in terms of operation robustness and user friendliness. Interferometry has opened a new observational window, enabling (sub)au-scale resolution of massive stars and direct measurements of orbital parameters, wind structures, and magnetic phenomena. This paper reviews recent advances in interferometric studies of massive stars, focusing on multiplicity, magnetism, and stellar winds.
Cite
@article{arxiv.2512.00444,
title = {Interferometry of Massive Stars: Multiplicity, Magnetism, and Stellar Winds},
author = {H. Sana E. Bordier and K. Deshmukh and A. J. Frost and A. Keskar and C. Lanthermann and R. R. Lefever and L. Mahy and A. A. C. Sander and T. Shenar and F. Tramper},
journal= {arXiv preprint arXiv:2512.00444},
year = {2025}
}
Comments
5 pages, 3 figures, 1 table, proceedings IAU 402