A new deepening of mass-radius empirical relation for main sequence stars
Abstract
In the following paper I have compared some typical mass-radius relations for main sequence stars by studying their level of agreement with DEBCat [https://doi.org/10.48550/arXiv.1411.1219], which is a recent catalogue by J. Southworth. Models chosen for testing were originally developed using older, smaller datasets than DEBCat. Each model follows a two-piece function structure, where each branch is a monomial power-law. This approach is motivated by theoretical considerations suggesting that low-mass and high-mass main sequence stars exhibit distinct behaviors in energy production and energy transport. Best level of agreement is found for Zamorano's model [https://doi.org/10.1007/bf00653969]. Also a new empirical relation is proposed by fitting a two-piece monomial power-law to DEBCat main sequence stars.
Cite
@article{arxiv.2508.08845,
title = {A new deepening of mass-radius empirical relation for main sequence stars},
author = {Salvatore Camposeo},
journal= {arXiv preprint arXiv:2508.08845},
year = {2025}
}
Comments
6 pages, 8 figures