A new deepening of mass-radius empirical relation for main sequence stars

In the following paper I have compared some typical mass-radius relations for main sequence stars by studying their level of agreement with DEBCat (J. Southworth, ASP Conf. Ser. 496 (2015), https://doi.org/10.48550/arXiv.1411.1219, https://www.astro.keele.ac.uk/jkt/debcat/debs.dat), which is a recen...

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Bibliographic Details
Main Author: Camposeo Salvatore
Format: Article
Language:English
Published: EDP Sciences 2025-01-01
Series:Emergent Scientist
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Online Access:https://emergent-scientist.edp-open.org/articles/emsci/full_html/2025/01/emsci240003/emsci240003.html
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