A dense $\mathbf{0.1 M_{\rm \odot}}$ star in a 51-minute orbital period eclipsing binary (2022)
Attributed to:
A consolidated grant for Sheffield Astrophysics 2021-2024
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2210.01809
Publication URI: https://arxiv.org/abs/2210.01809
Type: Other