Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars

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Table B.2.

Estimates of the ratio ζ between the mode inertia in the core and the total mode inertia, the mixed dipole mode widths Γ_n, 1, heights H_n, 1 and the pressure dipole mode widths for the stars KIC 6847371 at radial order n = 5 and 6, KIC 11032660 at n = 5 and 6, KIC 5461447 at n = 6, KIC 10857623 at n = 7, and KIC 6768042 at n = 7 and 8.

KIC	ν	ζ	Γ_n, 1		H_n, 1
	(μHz)		(nHz)	(μHz)	(ppm² μHz⁻¹)
6847371
	17.221	0.912	14.0	0.173	148 042
	17.312	0.933	8.9	0.134	119 977
	17.385	0.951	12.6	0.256	185 682
	17.444	0.961	12.8	0.330	132 426
	19.763	0.917	10.8	0.130	142 715
	19.836	0.900	13.5	0.135	185 918
	19.916	0.895	8.1	0.077	595 653
	19.981	0.908	17.5	0.190	419 721
	20.056	0.929	18.0	0.254	114 214
	20.121	0.944	9.1	0.163	272 377
	20.198	0.958	9.8	0.233	121 588

11032660
	18.054	0.901	9.1	0.092	66 802
	18.103	0.906	11.9	0.126	223 603
	18.176	0.922	14.7	0.189	223 744
	18.246	0.940	8.1 ^( * )	0.135	147 870
	18.300	0.956	8.5	0.191	149 941
	18.365	0.967	8.2	0.246	156 975
	20.836	0.892	12.3	0.113	106 265
	20.918	0.872	13.5	0.105	108 367
	20.999	0.881	8.2	0.069	231 565
	21.092	0.911	14.1	0.158	200 770

5461447
	21.715	0.947	13.9	0.263	65 961
	21.844	0.902	12.9	0.131	88 352
	22.007	0.835	15.5	0.094	39 418
	22.121	0.879	14.9	0.123	110 662
	22.218	0.925	13.7	0.183	118 859
	22.315	0.954	18.4	0.398	49 835

10857623
	20.745	0.924	9.7	0.127	63 988
	20.820	0.891	8.8	0.081	56 137
	20.913	0.848	7.8 ^( * )	0.051	140 292
	20.984	0.851	7.8 ^( * )	0.052	99 708
	21.065	0.882	12.1	0.103	163 003

6768042
	24.763	0.839	22.1	0.138	70 787
	24.873	0.832	7.9 ^( * )	0.047	80 691
	24.967	0.878	16.6	0.136	155 491
	25.088	0.928	16.3	0.225	101 482
	25.204	0.953	11.5	0.243	107 916
	27.504	0.927	10.5	0.143	35 161
	27.639	0.863	11.3	0.082	45 895
	27.780	0.790	14.5	0.069	87 860
	27.904	0.820	8.7	0.048	174 133
	28.037	0.899	14.0	0.138	45 005
	28.070	0.909	11.7	0.129	32 445
	28.182	0.940	15.3	0.254	39 866

Notes. The different estimates of are inferred from Eq. (12). For these particular stars, the term ζ is not derived from scaling relations as described in Sect. 3, but is extracted from the database of Mosser et al. (2018).

^( * )The measurement of the modes located at ν = 18.246 μHz (KIC 11032660), ν = 20.913 μHz and ν = 20.984 μHz (KIC 10857623), and ν = 24.873 μHz (KIC 6768042) are limited by the resolution.

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