Surface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)

Fuente: arXiv

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Bibliographic Details
Main Authors:	Xiong, Jianping, Cheng, Qiyuan, Chen, Xiaodian, Li, Jiao, Zhang, Xiaobin, Han, Zhanwen, Chen, Xuefei
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2503.11155