Table 2
X-ray luminosity in the 0.5–4.5 keV band, X-ray to bolometric luminosity ratio, effective temperatures, mass, radius, rotation period, and Rossby number of M34 target stars.
| Id. | 2XMM identifier | L X | L bol | LX/Lbol | T eff | M | R | P | Ro | Seq. |
| (1028 erg s-1) | (L⊙) | (10-3) | (K) | (M⊙) | (R⊙) | (d) | ||||
|
|
||||||||||
| 1 | J024126.0+424814. | 13.9 ± 2.9 | 0.977 | 0.037 ± 0.008 | 5927 | 1.08 | 0.94 | 3.99 | 0.31 | I |
| 2 | J024135.1+424103. | 76.4 ± 6.2 | 0.395 | 0.500 ± 0.041 | 5303 | (0.88) | 0.74 | 0.90 | 0.05 | C |
| 3 | J024136.6+425020. | 72.3 ± 5.6 | 0.365 | 0.518 ± 0.040 | 5231 | 0.89 | 0.74 | 2.80 | 0.16 | G |
| 4 | J024138.2+424403. | 2.1 ± 1.5 | 0.578 | 0.010 ± 0.007 | 5470 | (0.93) | 0.85 | 5.99 | 0.37 | I |
| 5 | J024138.5+423903. | 15.0 ± 3.6 | 0.870 | 0.045 ± 0.011 | 5784 | 1.04 | 0.93 | 4.37 | 0.32 | I |
| 6 | J024140.7+425446. | 13.0 ± 3.1 | 1.225 | 0.028 ± 0.007 | 5964 | 1.09 | 1.04 | 2.80 | 0.22 | I |
| 7 | J024143.9+424506. | 13.9 ± 2.6 | 0.073 | 0.496 ± 0.094 | 4251 | (0.63) | 0.50 | 0.59 | 0.02 | C |
| F4-0136 | J024147.3+424339. | 29.7 ± 3.5 | 1.044 | 0.074 ± 0.009 | 5855 | 1.05 | 0.99 | 2.87 (J10) | 0.21 | I |
| 8 | J024147.8+424121. | 20.9 ± 3.7 | 3.006 | 0.018 ± 0.003 | 6078 | 1.25 | 1.56 | 6.06 | 0.59 | I |
| F3-0413 | J024148.3+424933. | 22.5 ± 3.0 | 0.091 | 0.646 ± 0.085 | 4587 | (0.70) | 0.48 | 5.45 (I06) | 0.23 | G |
| 9 | J024148.7+424001. | 24.2 ± 4.1 | 0.134 | 0.472 ± 0.081 | 4640 | (0.71) | 0.57 | 4.83 | 0.21 | G |
| 10 | J024151.8+423822. | 11.9 ± 3.6 | 0.082 | 0.379 ± 0.115 | 4349 | (0.67) | 0.50 | 5.35 | 0.21 | G |
| M34-4-2215 | J024155.2+425031. | 10.1 ± 2.3 | 0.061 | 0.432 ± 0.097 | 3639 | (0.66) | (0.62) | 6.575 (I06) | 0.26 | G |
| 11 | J024157.3+430026. | 35.1 ± 5.8 | 0.193 | 0.475 ± 0.078 | 4862 | 0.80 | 0.62 | 1.13 | 0.06 | C |
| 12 | J024159.5+424102. | 16.5 ± 3.1 | 1.264 | 0.034 ± 0.006 | 5653 | 1.11 | 1.17 | 4.19 | 0.34 | I |
| M34-4-2015 | J024201.7+424158 | 9.4 ± 2.8 | 0.035 | 0.705 ± 0.212 | 3558 | (0.53) | (0.49) | 1.978 (I06) | 0.06 | C |
| 13 | J024205.8+424654. | 8.8 ± 2.1 | 0.462 | 0.050 ± 0.012 | 4862 | 0.87 | 0.96 | 8.27 | 0.47 | I |
| 14 | J024206.4+423621. | 22.2 ± 4.4 | 0.863 | 0.067 ± 0.013 | 5282 | 0.99 | 1.11 | 6.14 | 0.42 | I |
| 15 | J024208.3+423843. | 20.1 ± 4.0 | 1.271 | 0.041 ± 0.008 | 6117 | 1.14 | 1.00 | 2.71 | 0.23 | I |
| 16 | J024211.3+425035. | 18.6 ± 2.8 | 0.437 | 0.111 ± 0.016 | 5159 | 0.87 | 0.83 | 6.90 | 0.39 | I |
| 17 | J024213.9+425547. | 20.2 ± 3.4 | 0.584 | 0.090 ± 0.015 | 5359 | 0.92 | 0.89 | 4.65 | 0.28 | I |
| M34-4-1524 | J024217.2+424819. | 37.2 ± 3.4 | 0.183 | 0.532 ± 0.048 | 4508 | (0.75) | (0.70) | 1.179 (I06) | 0.05 | C |
| 18 | J024220.4+424905. | 4.5 ± 1.6 | 0.101 | 0.117 ± 0.042 | 4382 | (0.68) | 0.55 | 10.99 | 0.44 | I |
| 19 | J024231.8+423711. | 57.5 ± 9.0 | 0.119 | 1.263 ± 0.199 | 4605 | (0.74) | 0.54 | 1.07 | 0.05 | C |
| M34-4-1092 | J024232.5+424907. | 101.0 ± 5.7 | 0.274 | 0.964 ± 0.054 | 4612 | (0.86) | (0.82) | 0.678 (I06) | 0.04 | C |
| M34-1-1017 | J024234.8+423926 | 7.8 ± 2.9 | 0.024 | 0.845 ± 0.321 | 3380 | (0.49) | (0.45) | 3.633 (I06) | 0.10 | C |
| 20 | J024236.4+425433. | 65.8 ± 7.7 | 0.288 | 0.597 ± 0.069 | 5136 | (0.82) | 0.68 | 3.18 | 0.17 | G |
| M34-4-798 | J024241.9+424600. | 8.3 ± 2.3 | 0.029 | 0.746 ± 0.207 | 3403 | (0.53) | (0.49) | 7.322 (I06) | 0.22 | G |
| 21 | J024242.5+424031. | 47.0 ± 5.5 | 1.631 | 0.075 ± 0.009 | 6198 | 1.16 | 1.11 | 1.97 | 0.17 | I |
| 22 | J024243.6+425230. | 19.5 ± 3.5 | 0.178 | 0.286 ± 0.051 | 4518 | 0.73 | 0.69 | 10.75 | 0.48 | I |
| 23 | J024247.5+424545. | 34.7 ± 4.2 | 0.083 | 1.093 ± 0.133 | 4483 | (0.69) | 0.48 | 1.19 | 0.05 | C |
| 24 | J024249.1+424013. | 32.2 ± 5.0 | 0.134 | 0.629 ± 0.097 | 4786 | 0.79 | 0.53 | 1.50 | 0.07 | C |
| 25 | J024250.8+425807. | 54.0 ± 6.7 | 0.348 | 0.405 ± 0.050 | 5183 | (0.86) | 0.73 | 0.94 | 0.05 | C |
| 26 | J024251.7+424751. | 69.4 ± 6.2 | 1.493 | 0.121 ± 0.011 | 5751 | 1.15 | 1.23 | 3.67 | 0.31 | I |
| M34-4-316 | J024257.7+424147. | 36.9 ± 5.4 | 0.094 | 1.025 ± 0.150 | 3819 | (0.75) | (0.70) | 5.97 (I06) | 0.27 | G |
| 27 | J024258.2+425803. | 98.1 ± 10.8 | 0.275 | 0.932 ± 0.103 | 5136 | (0.84) | 0.66 | 1.55 | 0.08 | C |
| 28 | J024259.5+424821. | 15.3 ± 3.3 | 0.212 | 0.189 ± 0.041 | 4399 | 0.74 | 0.79 | 10.52 | 0.47 | I |
| M34-3-205 | J024300.1+425801. | 96.1 ± 11.0 | 0.182 | 1.380 ± 0.158 | 4474 | (0.76) | (0.71) | 0.789 (I06) | 0.04 | C |
| 29 | J024301.9+424651. | 12.7 ± 3.5 | 0.038 | 0.875 ± 0.243 | 4086 | 0.62 | 0.39 | 0.49 | 0.02 | C |
| 30 | J024320.9+424857. | 18.5 ± 4.9 | 0.155 | 0.312 ± 0.083 | 4518 | 0.72 | 0.64 | 8.85 | 0.38 | I |
| 31 | J024330.1+425307. | 63.9 ± 11.1 | 0.281 | 0.594 ± 0.103 | 5183 | 0.88 | 0.66 | 0.72 | 0.04 | C |
Notes. The rotation periods are from M 11 or otherwise from I06 or J10, as indicated between brackets in the corresponding column. Mass and radius estimates between bracketts are from I06. The last column gives the classification of each star as a member of the convective sequence (C), the interface sequence (I), or the gap (G).
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