Table 2.

Stellar parameters derived from Strömgren–Crawford photometry (Teff in Column 2), from BC (log(L in Column 4), and from isochrone fitting for the studied stars (Columns 3–10). Data for stellar luminosity, radius, and mass inferred from TIC 8 (Stassun et al. 2018) are shown for comparison in Columns 5, 7, 9, respectively. Data for the derived equatorial velocity are presented in the last two columns.

NameTeff (K)log glog(L/L)R (R)M (M)logAgeveq (km s−1)veq/vcrit (%)
HDThis studyThis studyThis studyTICThis studyTICThis studyTICThis studyThis studyThis study
PhotometryIsochroneBC cor.IsochroneIsochroneIsochrone
1084011489 ± 3164.17(4)1.92(1)2.035(35)2.336(2)2.550(80)2.878(2)3.09(39)8.175(8)56.33(5)11.62(1)
2292013714 ± 3863.95(2)2.60(3)2.424(320)3.55(2)4.06(1)8.071(1)45.5(3)9.74(7)
247127201 ± 2904.17(5)0.84(2)0.863(15)1.700(8)1.715(70)1.541(2)1.63(27)8.99(2)6.90(3)1.66(1)
381709493 ± 2933.81(2)1.92(3)2.006(34)3.38(2)3.354(142)2.649(3)2.56(35)8.639(3)61.8(4)16.0(1)
6340113201 ± 3804.20(2)2.22(3)2.475(9)3.464(4)7.87(1)51.9(2)10.03(5)
7452110474 ± 2853.82(2)2.13(3)3.54(1)2.994(5)8.488(3)25.4(7)6.33(2)
865927716 ± 3364.10(6)1.08(1)1.150(23)1.949(8)1.895(60)1.732(3)1.981(300)8.972(7)34.2(2)8.30(4)
NameTeff (K)log glog(L/L)R (R)M (M)logAgeveq (km s−1)veq/vcrit (%)
HDThis studyThis studyThis studyTICThis studyTICThis studyTICThis studyThis studyThis study
PhotometryIsochroneBC cor.IsochroneIsochroneIsochrone
1084011489 ± 3164.17(4)1.92(1)2.035(35)2.336(2)2.550(80)2.878(2)3.09(39)8.175(8)56.33(5)11.62(1)
2292013714 ± 3863.95(2)2.60(3)2.424(320)3.55(2)4.06(1)8.071(1)45.5(3)9.74(7)
247127201 ± 2904.17(5)0.84(2)0.863(15)1.700(8)1.715(70)1.541(2)1.63(27)8.99(2)6.90(3)1.66(1)
381709493 ± 2933.81(2)1.92(3)2.006(34)3.38(2)3.354(142)2.649(3)2.56(35)8.639(3)61.8(4)16.0(1)
6340113201 ± 3804.20(2)2.22(3)2.475(9)3.464(4)7.87(1)51.9(2)10.03(5)
7452110474 ± 2853.82(2)2.13(3)3.54(1)2.994(5)8.488(3)25.4(7)6.33(2)
865927716 ± 3364.10(6)1.08(1)1.150(23)1.949(8)1.895(60)1.732(3)1.981(300)8.972(7)34.2(2)8.30(4)
Table 2.

Stellar parameters derived from Strömgren–Crawford photometry (Teff in Column 2), from BC (log(L in Column 4), and from isochrone fitting for the studied stars (Columns 3–10). Data for stellar luminosity, radius, and mass inferred from TIC 8 (Stassun et al. 2018) are shown for comparison in Columns 5, 7, 9, respectively. Data for the derived equatorial velocity are presented in the last two columns.

NameTeff (K)log glog(L/L)R (R)M (M)logAgeveq (km s−1)veq/vcrit (%)
HDThis studyThis studyThis studyTICThis studyTICThis studyTICThis studyThis studyThis study
PhotometryIsochroneBC cor.IsochroneIsochroneIsochrone
1084011489 ± 3164.17(4)1.92(1)2.035(35)2.336(2)2.550(80)2.878(2)3.09(39)8.175(8)56.33(5)11.62(1)
2292013714 ± 3863.95(2)2.60(3)2.424(320)3.55(2)4.06(1)8.071(1)45.5(3)9.74(7)
247127201 ± 2904.17(5)0.84(2)0.863(15)1.700(8)1.715(70)1.541(2)1.63(27)8.99(2)6.90(3)1.66(1)
381709493 ± 2933.81(2)1.92(3)2.006(34)3.38(2)3.354(142)2.649(3)2.56(35)8.639(3)61.8(4)16.0(1)
6340113201 ± 3804.20(2)2.22(3)2.475(9)3.464(4)7.87(1)51.9(2)10.03(5)
7452110474 ± 2853.82(2)2.13(3)3.54(1)2.994(5)8.488(3)25.4(7)6.33(2)
865927716 ± 3364.10(6)1.08(1)1.150(23)1.949(8)1.895(60)1.732(3)1.981(300)8.972(7)34.2(2)8.30(4)
NameTeff (K)log glog(L/L)R (R)M (M)logAgeveq (km s−1)veq/vcrit (%)
HDThis studyThis studyThis studyTICThis studyTICThis studyTICThis studyThis studyThis study
PhotometryIsochroneBC cor.IsochroneIsochroneIsochrone
1084011489 ± 3164.17(4)1.92(1)2.035(35)2.336(2)2.550(80)2.878(2)3.09(39)8.175(8)56.33(5)11.62(1)
2292013714 ± 3863.95(2)2.60(3)2.424(320)3.55(2)4.06(1)8.071(1)45.5(3)9.74(7)
247127201 ± 2904.17(5)0.84(2)0.863(15)1.700(8)1.715(70)1.541(2)1.63(27)8.99(2)6.90(3)1.66(1)
381709493 ± 2933.81(2)1.92(3)2.006(34)3.38(2)3.354(142)2.649(3)2.56(35)8.639(3)61.8(4)16.0(1)
6340113201 ± 3804.20(2)2.22(3)2.475(9)3.464(4)7.87(1)51.9(2)10.03(5)
7452110474 ± 2853.82(2)2.13(3)3.54(1)2.994(5)8.488(3)25.4(7)6.33(2)
865927716 ± 3364.10(6)1.08(1)1.150(23)1.949(8)1.895(60)1.732(3)1.981(300)8.972(7)34.2(2)8.30(4)
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