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.
Name . | Teff (K) . | log g . | log(L⋆/L⊙) . | R (R⊙) . | M⋆ (M⊙) . | logAge . | veq (km s−1) . | veq/vcrit (%) . | |||
---|---|---|---|---|---|---|---|---|---|---|---|
HD . | This study . | This study . | This study . | TIC . | This study . | TIC . | This study . | TIC . | This study . | This study . | This study . |
. | Photometry . | Isochrone . | BC cor. . | . | Isochrone . | . | Isochrone . | . | Isochrone . | . | . |
10840 | 11489 ± 316 | 4.17(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) |
22920 | 13714 ± 386 | 3.95(2) | 2.60(3) | 2.424(320) | 3.55(2) | – | 4.06(1) | – | 8.071(1) | 45.5(3) | 9.74(7) |
24712 | 7201 ± 290 | 4.17(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) |
38170 | 9493 ± 293 | 3.81(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) |
63401 | 13201 ± 380 | 4.20(2) | 2.22(3) | – | 2.475(9) | – | 3.464(4) | – | 7.87(1) | 51.9(2) | 10.03(5) |
74521 | 10474 ± 285 | 3.82(2) | 2.13(3) | – | 3.54(1) | – | 2.994(5) | – | 8.488(3) | 25.4(7) | 6.33(2) |
86592 | 7716 ± 336 | 4.10(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) |
Name . | Teff (K) . | log g . | log(L⋆/L⊙) . | R (R⊙) . | M⋆ (M⊙) . | logAge . | veq (km s−1) . | veq/vcrit (%) . | |||
---|---|---|---|---|---|---|---|---|---|---|---|
HD . | This study . | This study . | This study . | TIC . | This study . | TIC . | This study . | TIC . | This study . | This study . | This study . |
. | Photometry . | Isochrone . | BC cor. . | . | Isochrone . | . | Isochrone . | . | Isochrone . | . | . |
10840 | 11489 ± 316 | 4.17(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) |
22920 | 13714 ± 386 | 3.95(2) | 2.60(3) | 2.424(320) | 3.55(2) | – | 4.06(1) | – | 8.071(1) | 45.5(3) | 9.74(7) |
24712 | 7201 ± 290 | 4.17(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) |
38170 | 9493 ± 293 | 3.81(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) |
63401 | 13201 ± 380 | 4.20(2) | 2.22(3) | – | 2.475(9) | – | 3.464(4) | – | 7.87(1) | 51.9(2) | 10.03(5) |
74521 | 10474 ± 285 | 3.82(2) | 2.13(3) | – | 3.54(1) | – | 2.994(5) | – | 8.488(3) | 25.4(7) | 6.33(2) |
86592 | 7716 ± 336 | 4.10(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) |
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.
Name . | Teff (K) . | log g . | log(L⋆/L⊙) . | R (R⊙) . | M⋆ (M⊙) . | logAge . | veq (km s−1) . | veq/vcrit (%) . | |||
---|---|---|---|---|---|---|---|---|---|---|---|
HD . | This study . | This study . | This study . | TIC . | This study . | TIC . | This study . | TIC . | This study . | This study . | This study . |
. | Photometry . | Isochrone . | BC cor. . | . | Isochrone . | . | Isochrone . | . | Isochrone . | . | . |
10840 | 11489 ± 316 | 4.17(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) |
22920 | 13714 ± 386 | 3.95(2) | 2.60(3) | 2.424(320) | 3.55(2) | – | 4.06(1) | – | 8.071(1) | 45.5(3) | 9.74(7) |
24712 | 7201 ± 290 | 4.17(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) |
38170 | 9493 ± 293 | 3.81(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) |
63401 | 13201 ± 380 | 4.20(2) | 2.22(3) | – | 2.475(9) | – | 3.464(4) | – | 7.87(1) | 51.9(2) | 10.03(5) |
74521 | 10474 ± 285 | 3.82(2) | 2.13(3) | – | 3.54(1) | – | 2.994(5) | – | 8.488(3) | 25.4(7) | 6.33(2) |
86592 | 7716 ± 336 | 4.10(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) |
Name . | Teff (K) . | log g . | log(L⋆/L⊙) . | R (R⊙) . | M⋆ (M⊙) . | logAge . | veq (km s−1) . | veq/vcrit (%) . | |||
---|---|---|---|---|---|---|---|---|---|---|---|
HD . | This study . | This study . | This study . | TIC . | This study . | TIC . | This study . | TIC . | This study . | This study . | This study . |
. | Photometry . | Isochrone . | BC cor. . | . | Isochrone . | . | Isochrone . | . | Isochrone . | . | . |
10840 | 11489 ± 316 | 4.17(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) |
22920 | 13714 ± 386 | 3.95(2) | 2.60(3) | 2.424(320) | 3.55(2) | – | 4.06(1) | – | 8.071(1) | 45.5(3) | 9.74(7) |
24712 | 7201 ± 290 | 4.17(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) |
38170 | 9493 ± 293 | 3.81(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) |
63401 | 13201 ± 380 | 4.20(2) | 2.22(3) | – | 2.475(9) | – | 3.464(4) | – | 7.87(1) | 51.9(2) | 10.03(5) |
74521 | 10474 ± 285 | 3.82(2) | 2.13(3) | – | 3.54(1) | – | 2.994(5) | – | 8.488(3) | 25.4(7) | 6.33(2) |
86592 | 7716 ± 336 | 4.10(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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