Evolution of the near-core rotation frequency of 2497 intermediate-mass stars from their dominant gravito-inertial mode

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Volume 695 (March 2025)

A&A, 695 (2025) A214

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202555611e]

Table 1.

Regression coefficients for y = a log T_eff + b.

y	a	b	r_Pearson	R²
f_dom	$22 . 2_{- 0.7}^{+ 0.7}$ $22.2_{-0.7}^{+0.7}$	$- 83 . 9_{- 2.5}^{+ 2.6}$ $-83.9_{-2.5}^{+2.6}$	0.426	0.162
$f_{dom}^{- 1}$ $f^{-1}_{\mathrm{dom}}$	$- 9 . 6_{- 0.3}^{+ 0.3}$ $-9.6_{-0.3}^{+0.3}$	$37 . 74_{- 1.11}^{+ 1.16}$ $37.74_{-1.11}^{+1.16}$	−0.426	0.171
¹⁰log(f_dom)	$6 . 5_{- 0.2}^{+ 0.2}$ $6.5_{-0.2}^{+0.2}$	$- 24 . 7_{- 0.7}^{+ 0.7}$ $-24.7_{-0.7}^{+0.7}$	0.426	0.169
f_rot	$18 . 6_{- 0.7}^{+ 0.7}$ $18.6_{-0.7}^{+0.7}$	$- 70 . 5_{- 2.7}^{+ 2.7}$ $-70.5_{-2.7}^{+2.7}$	0.400	0.155
$f_{rot}^{- 1}$ $f^{-1}_{\mathrm{rot}}$	$- 18 . 5_{- 0.8}^{+ 0.8}$ $-18.5_{-0.8}^{+0.8}$	$72 . 4_{- 2.9}^{+ 3.1}$ $72.4_{-2.9}^{+3.1}$	−0.400	0.166
¹⁰log(f_rot)	$8 . 3_{- 0.3}^{+ 0.3}$ $8.3_{-0.3}^{+0.3}$	$- 32 . 1_{- 1.2}^{+ 1.2}$ $-32.1_{-1.2}^{+1.2}$	0.400	0.164
Π₀(n + α_g)	$- 16 . 3_{- 1.5}^{+ 1.5}$ $-16.3_{-1.5}^{+1.5}$	$64 . 9_{- 5.8}^{+ 6.0}$ $64.9_{-5.8}^{+6.0}$	−0.250	0.187
(Π₀(n+α_g))⁻¹	$3 . 9_{- 0.4}^{+ 0.4}$ $3.9_{-0.4}^{+0.4}$	$- 14 . 5_{- 1.4}^{+ 1.4}$ $-14.5_{-1.4}^{+1.4}$	0.249	0.186
¹⁰log(Π₀(n+α_g))	$- 3 . 5_{- 0.3}^{+ 0.3}$ $-3.5_{-0.3}^{+0.3}$	$13 . 9_{- 1.2}^{+ 1.4}$ $13.9_{-1.2}^{+1.4}$	−0.249	0.188

Notes. All listed coefficients (a, b) differ significantly from zero at a p-value of 5%. Further, r_Pearson stands for the Pearson correlation coefficient and R² is the coefficient of determination.

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