Table 2
X-ray luminosities in the 0.5−4.5 keV band, bolometric luminosities, X-ray to bolometric luminosity ratios, effective temperatures, rotation periods, and Rossby numbers of M 35 cluster members stars not identified as binaries.
| 2XMM identifier | L X | L bol | LX/Lbol | T eff | P | Ro | Rotation |
| (1028 erg s-1) | (L⊙) | (10-3) | (K) | (d) | sequence | ||
|
|
|||||||
| J60844.9+241958. | 54 ± 13 | 0.99 | 0.14 ± 0.04 | 5386 | 3.720 | 0.29 | I |
| J60913.7+241545. | 155 ± 20 | 0.08 | 5.21 ± 0.68 | 4694 | 0.623 | 0.03 | C |
| J60900.5+241159. | 52 ± 15 | 1.34 | 0.10 ± 0.03 | 5684 | 0.560 | 0.05 | C |
| J60827.5+241238. | 75 ± 20 | 0.30 | 0.66 ± 0.17 | 5090 | 1.109 | 0.07 | C |
| J60928.7+242534. | 77 ± 19 | 0.50 | 0.40 ± 0.10 | 5413 | 1.275 | 0.10 | C |
| J60842.8+242939. | 170 ± 29 | 0.48 | 0.93 ± 0.16 | 5183 | 0.984 | 0.07 | C |
| J60908.6+242947. | 84 ± 23 | 0.04 | 5.71 ± 1.57 | 4217 | 0.651 | 0.02 | C |
| J60817.7+241225. | 155 ± 30 | 0.71 | 0.58 ± 0.11 | 5413 | 1.111 | 0.09 | C |
| J60923.5+243115. | 117 ± 30 | 0.47 | 0.65 ± 0.17 | 4922 | 1.288 | 0.08 | C |
| J60801.8+242645. | 91 ± 32 | 0.25 | 0.96 ± 0.33 | 5183 | 0.952 | 0.07 | C |
Notes.The last column gives the M09 classification of each star as a member of the convective sequence (C), the interface sequence (I), or the gap (g). X-ray luminosities were derived from X-ray fluxes (see Table 1) assuming a cluster distance of 762 pc. Uncertainties on stellar X-ray luminosities do not include the ±38% systematic error associated with the uncertainty on the cluster distance.
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