Table 5.
Metallicities, asteroseismic masses MAst. and evolutionary stages EAst. as determined by the reference given in the first column for 26 stars with asteroseismic as well as Bayesian stellar parameters and evolutionary stages available.
Ref. | Source Identifier | HIP | [Fe/H] | MAst. [M⊙] | EAst. | Mtrk. [M⊙] | Etrk. | Ptrk. |
---|---|---|---|---|---|---|---|---|
1 | KIC 03730953 | 93687 | −0.07 ± 0.03 | 1.97 ± 0.20a | HB |
![]() |
HB | 0.996 |
1 | KIC 04044238 | 94221 | 0.20 ± 0.03 | 1.06 ± 0.10a | HB |
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HB | 0.824 |
1 | KIC 05737655 | 98269 | −0.63 ± 0.03 | 0.78 ± 0.08a | HB |
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RGB | 0.683 |
1 | KIC 08813946 | 95005 | 0.09 ± 0.03 | 2.09 ± 0.21a | HB |
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HB | 0.997 |
1 | KIC 09705687 | 94976 | −0.20 ± 0.03 | 1.92 ± 0.19a | HB |
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HB | 0.981 |
1 | KIC 10323222 | 92885 | 0.04 ± 0.03 | 1.55 ± 0.16a | RGB |
![]() |
RGB | 0.999 |
1 | KIC 10404994 | 95687 | −0.06 ± 0.03 | 1.50 ± 0.15a | HB |
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HB | 0.990 |
1 | KIC 10716853 | 93376 | −0.08 ± 0.03 | 1.75 ± 0.18a | HB |
![]() |
HB | 0.990 |
1 | KIC 12884274 | 94896 | 0.11 ± 0.03 | 1.39 ± 0.14a | HB |
![]() |
HB | 0.977 |
2 | ∈ Tau | 20889 | 0.17 ± 0.06b | 2.40 ± 0.36 | HB |
![]() |
HB | 0.993 |
2 | β Gem | 37826 | 0.09 ± 0.04b | 1.73 ± 0.27 | HB |
![]() |
HB | 0.994 |
2 | 18 Del | 103527 | 0.07 ± 0.04c | 1.92 ± 0.30 | HB |
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RGB | 0.994 |
2 | γ Cep | 116727 | 0.13 ± 0.06 | 1.32 ± 0.20 | RGB |
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RGB | 1.000 |
2 | HD 5608 | 4552 | 0.12 ± 0.03 | 1.32 ± 0.21 | RGB | 1.574 ± 0.040 | RGB | 1.000 |
2 | κ CrB | 77655 | 0.13 ± 0.03 | 1.40 ± 0.21 | RGB |
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RGB | 1.000 |
2 | 6 Lyn | 31039 | −0.13 ± 0.02 | 1.37 ± 0.22 | RGB |
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RGB | 1.000 |
2 | HD 210702 | 109577 | 0.04 ± 0.03 | 1.47 ± 0.23 | RGB |
![]() |
RGB | 1.000 |
3 | HD 145428 | 79364 | −0.32 ± 0.12 |
![]() |
… |
![]() |
RGB | 1.000 |
3 | HD 4313 | 3574 | 0.05 ± 0.1 |
![]() |
… |
![]() |
RGB | 1.000 |
3 | HD 181342 | 95124 | 0.15 ± 0.1 |
![]() |
… | 1.380 ± 0.120 | RGB | 1.000 |
3 | HD 5319 | 4297 | 0.02 ± 0.1 |
![]() |
… |
![]() |
RGB | 1.000 |
3 | HD 185351 | 96459 | 0.00 ± 0.1b | 1.77 ± 0.08 | … |
![]() |
RGB | 1.000 |
3 | HD 212771 | 110813 | −0.1 ± 0.12 | 1.46 ± 0.09 | … |
![]() |
RGB | 1.000 |
3 | HD 106270 | 59625 | 0.06 ± 0.1 |
![]() |
… |
![]() |
RGB | 1.000 |
4 | γ Piscium | 114971 | −0.54 ± 0.10b | 1.00 ± 0.30d | HBe |
![]() |
HB | 0.907 |
4 | Θ1 Tauri | 20885 | 0.08 ± 0.10b | 2.70 ± 0.30 | HBe |
![]() |
HB | 0.997 |
Notes. We also provide Bayesian masses Mtrk. and evolutionary stages EB. together with their probability Ptrk.
No confidence interval provided; we estimated a 10% error from Fig. 10 in Takeda & Tajitsu (2015).
Metallicity from Hekker & Meléndez (2007).
Metallicity from Maldonado et al. (2013).
No mixed modes available, Beck et al. (2015) estimated the evolutionary stage from the frequency of the maximum oscillation power excess.
References. (1) Takeda & Tajitsu (2015); (2) Stello et al. (2017); (3) North et al. (2017); (4) Beck et al. (2015).
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