Low-mass stars dominate the hot (0.7 keV) Galactic X-ray emission

Fuente: arXiv

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Bibliographic Details
Main Authors:	Ponti, G., Yeung, M. C. H., Stel, G., Locatelli, N., Zheng, X., Stelzer, B., Merloni, A., Caramazza, M., Magaudda, E., Sasaki, M., Dennerl, K., Reiprich, T. H., Schwope, A., Becker, W., Freyberg, M.
Format:	Preprint
Published:	2026
Subjects:	Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2602.03941