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Can Radius-based Correction Factors be Generally Adopted for Asteroseismic Scaling Relations of Stellar Masses?

Authors: Zsóka Horváth, László Molnár, Csilla Kalup

Zsóka Horváth et al 2026 Research Notes of the AAS 10 .

Provider: AAS Journals

Caption: Figure 1.

Stellar masses inferred from the scaling relations in Equations (1)–(4) in three different sets. M_orig is from the relations without any ﹩{f}_{{\nu }_{{\rm{\max }}}}﹩ and f_Δν corrections; M_APOKASC uses correction factors derived from the APOKASC-3 catalog; and M_adj is after applying the alternative correction scheme to the APOKASC-3 factors proposed by K. Cao & M. H. Pinsonneault (2025).

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