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20242026
most citedSurface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)

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astro-ph.SR2025★ 1 cited

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

Jianping Xiong, Qiyuan Cheng, Xiaodian Chen +4

Aims. Asteroseismic radius and Gaia distance (ARD) method has been proposed to establish the SBCRs for late-type stars. Methods. We select Kepler RGB stars with high-precision aste…