Acta Physica Sinica, Volume. 68, Issue 21, 219701-1(2019)
Figures & Tables(13)
Fig. 1. (a) Variations of equatorial velocity in single star models; (b) variations of equatorial velocity in binary star models. Hollow diamonds denote the end of main sequence; hollow circles stand for the beginning of helium burning; solid circles denote the end of helium burning; hollow squares represent the beginning of carbon burning; solid squares represent the end of carbon burning(a)单星模型赤道转动速度随时间的变化; (b)双星模型赤道转动速度随时间的变化; 其中, 空心菱形为主序结束, 空心圆圈为中心氦开始燃烧, 实心圆圈为中心氦燃烧结束, 空心正方形为中心碳开始燃烧, 实心正方形是中心碳燃烧结束
Fig. 2. (a) Stellar mass and its mass of convective core vary with evolutionary time for the models of single star; (b) stellar mass and its mass of convective core vary with evolutionary time for the models of binary star(a) 各种单星模型的质量(实线)和其对应的对流核的质量(划线)随时间的变化; (b) 各种双星模型的质量(实线)和其对应的对流核的质量(划线)随时间的变化
Fig. 3. (a) Surface nitrogen abundance vary with evolutionary time for the models of single star; (b) surface nitrogen abundance vary with evolutionary time for the models of binary star; (c) surface helium abundance vary with central helium for the models of single stars and binary star(a)单星模型中恒星表面氮丰度随时间的演化; (b)双星模型中两子星表面氮丰度随时间的演化; (c) 主序阶段, 单星和双星模型的表面氦质量丰度随中心氦质量丰度的变化
Fig. 4. (a) Evolution as a function of the actual mass of the abundances (in mass fraction) of different elements at the surface of a non-rotating single model S1; (b) evolution as a function of the actual mass of the abundances (in mass fraction) of different elements at the surface of a rotating single model S6; (c) evolution as a function of the actual mass of the abundances (in mass fraction) of different elements at the surface of the primary star of model B1; (d) evolution as a function of the actual mass of the abundances (in mass fraction) of different elements at the surface of the primary star of model B2(a) 单星非转动S1模型表面各种元素的质量丰度的对数值随时间的演化; (b) 单星转动S6模型表面各种元素的质量丰度的对数值随时间的演化; (c) 双星非转动B1模型中的主星表面各种元素的质量丰度的对数值随时间的演化; (d) 双星转动模型B2中的主星表面各种元素的质量丰度的对数值随时间的演化
Fig. 5. Rate of mass transfer during Roche lobe overflow vary with evolutionary time for the models of binary star双星模型洛希瓣物质交换率随时间的演化
Fig. 6. (a) Evolutionary tracks in HR diagram for single stars; (b) evolutionary tracks in HR diagram for binaries(a) 单星模型在赫罗图中演化; (b) 双星模型中的主星在赫罗图中的演化; 双星模型的初始偏心率为0
Fig. 7. (a) Surface mass fraction of hydrogen varies with central helium mass fraction in models of single star; (b) surface effective temperature varies with central helium mass fraction in models of single star; (c) surface mass fraction of hydrogen varies with central helium mass fraction in models of binary star; (d) surface effective temperature varies with central helium mass fraction in models of of binary star(a) 单星模型表面氢的质量丰度随中心氦质量丰度的变化; (b) 单星模型表面有效温度随中心氦质量丰度的变化; (c) 双星模型表面氢的质量丰度随中心氦质量丰度的变化; (d) 双星模型表面有效温度随中心氦质量丰度的变化
Table 1. Criteria for classification of WR stars
View tableView in ArticleTable 1. Criteria for classification of WR stars
0.45 WR星的类型 判定依据 注: $T_{\rm eff}$ ${X_{i} }/{X_{j} }$ $\rm ({C+O})/{He}$ O型星 $\log (T_{\rm eff})>4.5$ WNL型星 $\log (T_{\rm eff})>4.0$ $X_{\rm H} <0.3$ WNE型星 $X_{\rm H} <10^{-5}$ $X_{\rm C} WNC型星 $\dfrac{X_{\rm C}}{X_{\rm N}}>0.1$ $\dfrac{X_{\rm C}}{X_{\rm N}}<10$ WC型星 $X_{\rm C}>X_{\rm N}$ $\rm \dfrac{C+O}{He}<1$ WO型星 $X_{\rm C}>X_{\rm N}$ $\rm \dfrac{C+O}{He}>1$
Table 2. Initial parameters for single stars and binaries
View tableView in ArticleTable 2. Initial parameters for single stars and binaries
Models $M_1/M_\odot$ $M_2/M_\odot$ $Z$ $\alpha$ $P_{\rm orb, ini}$ $V_{\rm ini, 1}$ $V_{\rm ini, 2}$ 注: B为双星系统, S为单星; $M_1$ $M_2$ $M_{\odot}$ $\alpha$ $P_{\rm orb, ini}$ $V_{\rm ini, 1}$ $V_{\rm ini, 2}$ S1 60 — 0.014 0.0385 — 0 — S2 60 — 0.014 0.0385 — 300 — S3 60 — 0.014 0.0385 — 600 — S4 40 — 0.014 0.0385 — 300 — S5 60 — 0.0021 0.0385 — 300 — S6 60 — 0.0021 0.0385 — 600 — B1 60 40 0.014 0.0385 3.0 0 0 B2 60 40 0.014 0.0385 3.0 300 300 B3 60 40 0.014 0.0385 3.0 600 600 B4 60 40 0.014 0.0385 40.0 300 300 B5 60 40 0.0021 0.0385 3.0 300 300
Table 3. Parameters for single star at different evolutionary stages
View tableView in ArticleTable 3. Parameters for single star at different evolutionary stages
Sequence Age/Myr $M/M_{\odot}$ $\log T_{\rm eff}$ $\log ({L_{1}}/{L_{\odot}})$ $\rm [N/H]$ $V_{\rm eq}$ $\log T_{\rm c}$ $\log \rho_{\rm c}$ 注: ZAMS为零龄主序; TAMS表示主序结束; BCHEB为中心氦核开始燃烧; ECHEB为中心氦核结束燃烧; BCCB 为中心碳核开始燃烧; CCB为中心碳核结束燃烧. ZAMS S1 0.0000 60.00 4.68 5.72 7.84 0.00 7.60 0.31 S2 0.0000 60.00 4.66 5.70 7.84 300.00 7.59 0.29 S3 0.0000 60.00 4.63 5.64 7.84 600.00 7.58 0.26 S4 0.0000 40.00 4.62 5.34 7.84 300.00 7.57 0.40 S5 0.0000 60.00 4.67 5.74 6.99 300.00 7.57 0.24 S6 0.0000 60.00 4.65 5.70 6.99 600.00 7.56 0.21 TAMS S1 3.9511 42.02 4.42 5.98 9.01 0.00 7.81 0.91 S2 4.1537 44.42 4.46 6.00 8.96 18.07 7.81 0.90 S3 4.5124 37.75 4.69 5.98 9.29 18.66 7.81 0.92 S4 5.3408 31.87 4.22 5.70 8.63 1.42 7.79 1.00 S5 4.3346 54.56 4.29 6.05 7.96 7.21 7.87 1.05 S6 5.0531 34.52 4.88 5.99 8.96 25.65 7.86 1.10 BCHEB S1 3.9550 42.01 4.46 6.00 9.01 0.00 7.98 1.43 S2 4.1574 44.40 4.51 6.02 8.98 19.75 7.98 1.42 S3 4.5162 37.62 4.77 6.01 9.30 25.72 7.98 1.45 S4 5.3453 31.83 4.25 5.72 8.63 1.37 7.96 1.51 S5 4.3383 54.53 4.31 6.06 7.96 7.28 8.03 1.55 S6 5.0570 34.44 4.96 6.02 8.97 36.78 8.03 1.60 ECHEB S1 4.3054 25.27 5.21 5.99 23.45 0.00 8.53 3.13 S2 4.5120 25.94 5.21 6.00 23.02 158.64 8.53 3.13 S3 4.8924 16.90 5.20 5.74 24.64 76.49 8.51 3.22 S4 5.7771 15.57 5.35 5.79 25.17 327.58 8.88 4.59 S5 4.6825 39.56 4.45 6.19 8.45 5.98 8.54 3.07 S6 5.4231 18.20 5.21 5.79 28.82 49.92 8.52 3.21 BCCB S1 4.3099 25.16 5.33 6.06 16.72 0.00 8.83 4.14 S2 4.5167 25.81 5.34 6.07 19.18 286.44 8.85 4.24 S3 4.8980 16.80 5.34 5.83 20.60 149.13 8.86 4.45 S4 5.7772 15.57 5.36 5.79 25.28 334.92 8.92 4.78 S5 4.6870 39.45 4.46 6.25 8.57 37.32 8.84 4.12 S6 5.4284 18.10 5.34 5.87 20.66 94.78 8.85 4.35 ECCB S1 4.3100 25.15 5.42 6.09 18.59 0.00 9.07 5.25 S2 4.5167 25.81 5.42 6.10 18.47 313.57 9.06 5.19 S3 4.8981 16.80 5.41 5.86 20.55 157.94 9.06 5.40 S4 5.7772 15.57 5.40 5.81 25.43 367.73 9.03 5.33 S5 — — — — — — — — S6 5.4285 18.10 5.41 5.90 20.90 97.57 9.05 5.34
Table 4. Evolutionary parameters for binary star at different stages.
View tableView in ArticleTable 4. Evolutionary parameters for binary star at different stages.
Sequence Age /Myr $P_{\rm orb}$ /d $M_{1}/M_{\odot}$ $M_{2}/M_{\odot}$ $\log(T_{\rm eff, 1})$ /K $\log \Big(\dfrac{L_{1}}{L_{\odot} }\Big)$ $\log(T_{\rm eff, 2})$ /K $\log \Big(\dfrac{L_{2}}{L_{\odot} }\Big)$ > $\Big[\rm \dfrac{N_{1}}{H}\Big]$ > $\Big[\rm \dfrac{N_{2}}{H}\Big]$ $V_{\rm eq1}$ km·s–1 $V_{\rm eq2}$ km·s–1 $\log T_{\rm c}$ K $\log \rho_{\rm c}$ g·cm–3 ZAMS B1 0.0000 3.00 60.00 40.00 4.68 5.71 4.64 5.36 7.84 7.84 0.00 0.00 7.62 0.37 B2 0.0000 3.00 60.00 40.00 4.67 5.70 4.63 5.34 7.84 7.84 288.35 294.86 7.61 0.35 B3 0.0000 3.00 60.00 40.00 4.64 5.65 4.59 5.27 7.84 7.84 566.93 581.75 7.60 0.32 B4 0.0000 40.00 60.00 40.00 4.67 5.70 4.63 5.34 7.84 7.84 288.35 294.86 7.61 0.35 B5 0.0000 3.00 60.00 40.00 4.69 5.66 4.65 5.29 6.99 6.99 306.83 301.14 7.66 0.50 BTM1 B1 2.6862 3.60 53.01 38.15 4.59 5.84 4.59 5.48 7.84 7.84 0.00 0.00 7.64 0.39 B2 2.6314 3.63 51.90 38.00 4.59 5.82 4.59 5.47 8.25 7.94 250.24 162.73 7.63 0.39 B3 2.7810 4.12 51.34 37.86 4.57 5.83 4.59 5.48 8.22 7.96 238.80 146.79 7.64 0.40 B4 4.1328 63.17 43.82 35.94 4.23 6.02 4.49 5.56 9.05 8.69 35.18 120.39 8.24 2.26 B5 2.9131 3.25 57.69 39.46 4.60 5.86 4.61 5.47 7.34 7.07 270.95 164.95 7.68 0.52 ETM1 B1 3.8956 4.25 36.84 43.77 4.62 5.90 4.57 5.67 9.20 8.18 0.00 0.00 7.70 0.61 B2 2.7305 3.41 45.44 43.82 4.60 5.78 4.61 5.57 8.66 8.26 239.26 177.55 7.63 0.42 B3 2.9777 3.92 44.57 43.27 4.59 5.81 4.60 5.58 8.83 8.25 226.58 161.96 7.64 0.44 B4 4.1426 65.47 36.94 36.00 4.27 6.10 4.49 5.56 9.26 8.67 73.07 330.19 8.31 2.47 B5 3.9817 3.61 38.02 51.22 4.63 5.87 4.65 5.73 8.27 7.82 217.02 168.84 7.72 0.69 TAMS B1 4.0397 4.65 33.60 43.48 4.68 5.91 4.56 5.68 9.30 8.18 0.00 0.00 7.81 0.95 B2 4.1254 5.13 25.57 43.47 4.83 5.79 4.53 5.69 9.86 8.41 20.52 193.13 7.80 0.99 B3 4.0832 5.43 27.93 43.40 4.81 5.84 4.54 5.68 9.66 8.44 19.99 174.17 7.80 0.97 B4 4.0693 62.61 44.06 36.03 4.41 5.97 4.54 5.56 8.82 8.63 6.63 68.60 7.72 0.65 B5 4.3382 3.81 34.79 50.91 4.68 5.92 4.63 5.75 8.44 7.81 169.76 181.54 7.86 1.10 BCHEB B1 4.0409 4.65 33.57 43.48 4.69 5.91 4.56 5.68 9.30 8.18 0.00 0.00 7.82 0.99 B2 4.1297 5.15 25.44 43.46 4.92 5.82 4.53 5.69 9.87 8.41 30.07 192.49 7.97 1.52 B3 4.0874 5.45 27.80 43.39 4.90 5.87 4.54 5.68 9.68 8.44 29.48 173.40 7.98 1.50 B4 4.1281 63.03 43.88 35.95 4.48 5.99 4.53 5.56 9.04 8.63 4.75 60.68 7.91 1.21 B5 4.3422 3.82 34.74 50.91 4.75 5.94 4.63 5.76 8.44 7.81 149.04 181.17 8.02 1.60 BMT2 B1 4.0474 4.67 33.39 43.47 4.63 6.00 4.58 5.69 9.30 9.30 0.00 0.00 8.24 2.29 B2 3.1581 3.55 43.04 43.10 4.61 5.81 4.59 5.59 8.99 8.19 231.13 191.20 7.64 0.45 B3 3.1290 3.97 43.65 43.04 4.59 5.82 4.59 5.58 8.93 8.23 223.55 166.73 7.64 0.45 B4 — — — — — — — — — — — — — — B5 4.3460 3.84 34.70 50.90 4.66 5.99 4.63 5.76 8.44 7.81 187.54 180.93 8.26 2.34 EMT2 B1 4.0562 5.13 30.44 45.39 4.65 6.06 4.62 5.72 9.48 8.74 0.00 0.00 8.31 2.49 B2 3.5409 3.78 37.67 44.95 4.61 5.82 4.59 5.65 9.06 8.42 212.81 195.54 7.66 0.51 B3 3.6151 4.27 37.66 44.50 4.60 5.84 4.58 5.65 9.07 8.44 203.84 175.46 7.66 0.52 B4 — — — — — — — — — — — — — — B5 4.3517 4.25 31.33 51.54 4.67 6.05 4.64 5.77 8.60 7.91 174.27 292.23 8.31 2.49 ECHEB B1 4.4454 8.50 14.60 44.32 5.30 5.71 4.57 5.75 25.43 8.65 0.00 0.00 8.74 3.96 B2 4.5716 8.31 11.27 42.40 5.27 5.52 4.45 5.73 24.26 8.41 58.94 181.80 8.70 3.93 B3 4.5155 9.20 12.05 42.46 5.27 5.56 4.47 5.71 24.15 8.44 52.74 142.55 8.68 3.83 B4 4.3645 94.44 25.01 35.66 5.14 5.92 4.50 5.58 24.02 8.65 0.32 127.17 8.37 2.68 B5 4.6953 5.16 24.36 51.19 5.18 5.95 4.61 5.80 27.78 7.85 6.01 149.71 8.48 2.99 BCCB B1 4.4468 8.51 14.58 44.31 5.35 5.75 4.57 5.75 24.91 8.65 0.00 0.00 8.89 4.66 B2 4.5741 8.32 11.24 42.40 5.33 5.58 4.45 5.73 23.39 8.41 67.64 179.57 8.85 4.60 B3 4.5184 9.22 12.02 42.45 5.34 5.62 4.47 5.71 24.42 8.44 62.74 140.22 8.88 4.71 B4 4.4963 110.76 20.53 35.48 5.36 5.95 4.48 5.59 24.89 8.65 0.56 99.94 8.90 4.56 B5 4.7078 5.25 23.75 51.18 5.37 6.03 4.61 5.80 23.51 7.85 10.68 146.97 8.92 4.63 ECCB B1 4.4469 8.51 14.58 44.31 5.41 5.77 4.57 5.75 24.88 8.65 0.00 0.00 9.04 5.38 B2 4.5743 8.32 11.24 42.40 5.37 5.60 4.45 5.73 22.95 8.41 66.77 173.97 9.01 5.44 B3 4.5185 9.22 12.01 42.45 5.38 5.64 4.47 5.71 24.41 8.44 63.39 136.75 9.01 5.41 B4 4.4963 110.77 20.53 35.48 5.42 5.97 4.48 5.59 24.88 8.65 0.67 98.21 9.05 5.22 B5 4.7078 5.25 23.75 51.18 5.42 6.04 4.61 5.80 23.50 7.85 12.57 144.92 9.05 5.18
Table 5. Mass fraction of various chemical elements at stellar surfaces at different stages in models S1, S2, and S6
View tableView in ArticleTable 5. Mass fraction of various chemical elements at stellar surfaces at different stages in models S1, S2, and S6
Sequence Age/Myr $M_1/M_{\odot}$ log( $X_{\rm ^{1}H}$ log( $X_{\rm ^{4}He}$ log( $X_{\rm ^{12}C}$ log( $X_{\rm ^{14}N}$ log( $X_{\rm ^{16}O}$ log( $X_{\rm ^{19}F}$ log( $X_{\rm ^{20}Ne}$ log( $X_{\rm ^{22}Ne}$ $X_{\rm ^{26}Al}$ ZAMS S1 0.0000 60.00 –0.14 –0.58 –2.62 –3.15 –2.18 –6.46 –2.87 –3.96 0 S2 0.0000 60.00 –0.14 –0.58 –2.62 –3.15 –2.18 –6.46 –2.87 –3.96 0 S6 0.0000 60.00 –0.12 –0.63 –3.45 –3.98 –3.01 –7.28 –3.69 –4.78 0 TAMS S1 3.9511 42.02 –0.23 –0.40 –3.91 –2.08 –3.07 –9.23 –2.87 –6.77 9.77 × 10–6 S2 4.1537 44.42 –0.22 –0.42 –3.70 –2.11 –2.86 –7.86 –2.87 –5.37 4.57 × 10–6 S6 5.0531 34.52 –0.99 –0.05 –4.56 –2.88 –4.60 –10.46 –3.83 –7.51 4.36 × 10–6 BCHEB S1 3.9550 42.01 –0.23 –0.40 –3.91 –2.08 –3.07 –9.23 –2.87 –6.77 9.77 × 10–6 S2 4.1574 44.40 –0.22 –0.41 –3.77 –2.10 –2.91 –8.07 –2.87 –5.58 4.89 × 10–6 S6 5.0570 34.44 –0.99 –0.05 –4.56 –2.88 –4.60 –10.46 –3.83 –7.51 4.36 × 10–6 WNL S1 4.1147 34.94 –0.58 –0.14 –3.87 –2.06 –3.63 –9.72 –2.88 –6.53 4.16 × 10–5 S2 4.3343 36.29 –0.57 –0.14 –3.82 –2.06 –3.59 –9.67 –2.88 –6.45 3.54 × 10–5 S6 4.1796 48.34 –0.52 –0.16 –4.60 –2.88 –4.55 –10.50 –3.79 –7.50 4.46 × 10–6 WNE S1 4.1801 31.26 –5.02 –0.01 –3.73 –2.05 –3.77 –9.61 –2.89 –6.56 5.62 × 10–5 S2 — — — — — — — — — — — S6 — — — — — — — — — — — WC S1 4.2217 28.36 –21.87 –0.51 –0.34 –17.12 –0.68 –4.71 –2.80 –1.88 1.12 × 10–15 S2 4.4173 30.79 –5.22 –0.02 –1.50 –2.06 –2.05 –5.72 –2.89 –2.91 4.67 × 10–5 S6 5.2107 29.81 –5.80 –0.02 –1.37 –2.89 –2.52 –6.15 –3.84 –3.38 3.80 × 10–6 WO S1 4.2569 26.70 –21.35 –0.65 –0.34 –16.95 –0.52 –4.72 –2.70 –1.89 2.57 × 10–15 S2 4.4302 28.58 –17.68 –0.71 –0.36 –5.17 –0.45 –4.72 –2.63 –1.91 4.16 × 10–8 S6 5.3898 18.84 –29.68 –0.64 –0.32 –17.99 –0.55 –5.48 –3.51 –2.71 8.51 × 10–17 ECHEB S1 4.3054 25.27 –29.41 –0.77 –0.37 –16.81 –0.41 –4.72 –2.59 –1.91 5.01 × 10–15 S2 4.5120 25.94 –28.78 –0.82 –0.39 –16.61 –0.38 –4.72 –2.54 –1.93 7.07 × 10–15 S6 5.4231 18.20 –35.90 –0.71 –0.33 –17.93 –0.48 –5.48 –3.43 –2.72 1.14 × 10–16 BCCB S1 4.3099 25.16 –22.67 –0.79 –0.37 –16.80 –0.40 –4.73 –2.58 –1.92 5.37 × 10–15 S2 4.5167 25.81 –24.97 –0.83 –0.40 –16.64 –0.37 –4.72 –2.52 –1.93 7.58 × 10–15 S6 5.4284 18.10 –27.74 –0.72 –0.33 –17.93 –0.47 –5.48 –3.41 –2.72 1.54 × 10–16 ECCB S1 4.3100 25.15 –24.54 –0.79 –0.37 –16.80 –0.40 –4.73 –2.58 –1.92 5.37 × 10–15 S2 4.5167 25.81 –24.26 –0.83 –0.40 –16.64 –0.37 –4.72 –2.52 –1.93 7.76 × 10–15 S6 5.4285 18.10 –27.99 –0.72 –0.33 –17.93 –0.47 –5.48 –3.41 –2.72 1.54 × 10–16
Table 6. Mass fraction of various chemical elements at the surfaces of the primary star at different stages in models B1 and B2
View tableView in ArticleTable 6. Mass fraction of various chemical elements at the surfaces of the primary star at different stages in models B1 and B2
Sequence Age/Myr $M_1/M_{\odot}$ log( $X_{\rm ^{1}H}$ log( $X_{\rm ^{4}He}$ log( $X_{\rm ^{12}C}$ log( $X_{\rm ^{14}N}$ log( $X_{\rm ^{16}O}$ log( $X_{\rm ^{19}F}$ log( $X_{\rm ^{20}Ne}$ log( $X_{\rm ^{22}Ne}$ $X_{\rm ^{26}Al}$ ZAMS B1 0.0000 60.00 –0.14 –0.58 –2.62 –3.15 –2.18 –6.46 –2.87 –3.96 0 B2 0.0000 60.00 –0.14 –0.58 –2.62 –3.15 –2.18 –6.46 –2.87 –3.96 0 BTM1 B1 2.6862 53.01 –0.14 –0.58 –2.62 –3.15 –2.18 –6.54 –2.95 –4.04 3.31 × 1021 B2 2.6314 51.90 –0.14 –0.58 –2.76 –2.74 –2.21 –6.66 –2.95 –4.16 3.38 × 10–7 ETM1 B1 3.8956 36.84 –0.40 –0.23 –3.87 –2.06 –3.56 –9.69 –2.96 –6.62 1.81 × 10–5 B2 2.7305 45.44 –0.16 –0.53 –3.02 –2.36 –2.38 –6.94 –2.95 –4.45 3.89 × 10–6 ECHB B1 4.0397 33.60 –0.50 –0.18 –3.85 –2.05 –3.61 –9.72 –2.96 –6.61 2.45 × 10–5 B2 4.1254 25.57 –1.06 –0.05 –3.80 –2.05 –3.67 –9.68 –2.96 –6.63 4.16 × 10–5 BCHEB B1 4.0409 33.57 –0.50 –0.18 –3.85 –2.05 –3.61 –9.72 –2.96 –6.61 2.45 × 10–5 B2 4.1297 25.44 –1.07 –0.05 –3.80 –2.05 –3.67 –9.68 –2.96 –6.63 4.16 × 10–5 BMT2 B1 4.0474 33.39 –0.50 –0.18 –3.85 –2.05 –3.61 –9.72 –2.96 –6.61 2.51 × 10–5 B2 3.1581 43.04 –0.24 –0.39 –3.80 –2.09 –2.95 –8.24 –2.95 –5.76 1.31 × 10–5 WNL B1 4.0480 32.78 –0.52 –0.16 –3.85 –2.05 –3.61 –9.73 –2.96 –6.62 2.81 × 10–5 B2 3.8633 32.25 –0.52 –0.16 –3.85 –2.05 –3.61 –9.72 –2.96 –6.60 2.95 × 10–5 EMT2 B1 4.0562 30.44 –0.68 –0.11 –3.84 –2.05 –3.64 –9.72 –2.96 –6.60 3.89 × 10–5 B2 3.5409 37.67 –0.28 –0.34 –3.86 –2.07 –3.16 –8.72 –2.95 –6.19 1.41 × 10–5 WNE B1 4.1344 26.76 –5.00 –0.01 –3.73 –2.05 –3.76 –9.59 –2.97 –6.65 4.78 × 10–5 B2 4.2129 22.30 –5.18 –0.01 –3.68 –2.06 –3.74 –9.45 –2.97 –6.52 4.78 × 10–5 WC B1 4.1976 23.92 –28.45 –0.09 –0.80 –14.82 –2.17 –4.58 –2.97 –1.87 6.45 × 10–17 B2 4.2498 21.01 –10.94 –0.01 –2.05 –2.10 –3.40 –5.62 –2.97 –2.91 4.36 × 10–5 WO B1 4.4339 14.75 –31.67 –0.64 –0.31 –17.28 –0.58 –4.59 –2.85 –1.88 5.62 × 10–5 B2 — — — — — — — — — — — ECHEB B1 4.4454 14.60 –31.77 –0.70 –0.31 –17.19 –0.53 –4.59 –2.82 –1.89 7.76 × 10–16 B2 4.5716 11.27 –30.86 –0.60 –0.30 –17.45 –0.65 –4.58 –2.90 –1.88 2.45 × 10–16 BCCB B1 4.4468 14.58 –31.25 –0.70 –0.31 –17.19 –0.53 –4.59 –2.82 –1.89 7.76 × 10–16 B2 4.5741 11.24 –29.98 –0.61 –0.30 –17.44 –0.64 –4.58 –2.90 –1.88 2.51 × 10–16 ECCB B1 4.4469 14.58 –31.22 –0.70 –0.31 –17.19 –0.53 –4.59 –2.82 –1.89 7.76 × 10–16 B2 4.5743 11.24 –29.54 –0.61 –0.30 –17.44 –0.64 –4.58 –2.90 –1.88 2.51 × 10–16
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Wei-Guo Peng, Han-Feng Song, Qiong Zhan, Xing-Hua Wu, Jiang-Hong Jing.
Paper Information
Received: Jul. 8, 2019
Accepted: --
Published Online: Sep. 17, 2020
The Author Email: Zhan Qiong (zhanqiong1108@163.com)
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