Table 1
X-ray fluxes, rotation periods, and photometric indices of X-ray emitting stars in M 35.
| 2XMM identifier | X-ray flux | P | V 0 | (B − V)0 | Phot. | Spect. | Comments | |
| (10-15 erg s-1 cm-2) | (days) | Mmb. (1) | Mmb. (2) | |||||
|
|
||||||||
| J060902.4+241952 | 12.7 ± 2.1 | 1.101 | 15.68 | 0.89 | PSM | BLM | ||
| J060844.9+241958 | 7.7 ± 1.9 | 3.720 | 14.34 | 0.76 | PSM | SM | ||
| J060903.5+241724 | 7.1 ± 1.7 | 2.400 | 15.35 | 0.90 | PSM | BM | SB1 | |
| J060902.0+241633 | 8.0 ± 1.8 | 8.820 | 15.76 | 0.93 | PM | SN | ||
| J060913.7+241545 | 22.4 ± 2.9 | 0.623 | 17.40 | 1.08 | PM | |||
| J060921.9+241850 | 15.9 ± 2.5 | 1.329 | 15.25 | 0.92 | PSM | SN | ||
| J060900.5+241159 | 7.5 ± 2.2 | 0.560 | 13.94 | 0.66 | PSM | SM | ||
| J060827.5+241238 | 10.8 ± 2.9 | 1.109 | 15.74 | 0.88 | PSM | SM | ||
| J060812.9+241746 | 9.8 ± 2.8 | 0.353 | 15.97 | 0.88 | PM | SN | ||
| J060928.7+242534 | 11.1 ± 2.7 | 1.275 | 15.07 | 0.75 | PSM | SM | ||
| J060842.8+242939 | 24.5 ± 4.1 | 0.984 | 15.19 | 0.84 | PSM | SM | ||
| J060809.9+242059 | 17.1 ± 3.5 | 1.231 | 14.11 | 0.81 | PNM | U | ||
| J060908.6+242947 | 12.2 ± 3.4 | 0.651 | 18.54 | 1.36 | PM | |||
| J060915.5+241041 | 29.0 ± 4.1 | 3.710 | 14.87 | 0.83 | PSM | BN | SB1 | |
| J060817.7+241225 | 22.4 ± 4.3 | 1.111 | 14.70 | 0.75 | PSM | SM | ||
| J060837.7+243146 | 9.2 ± 3.1 | 2.333 | 15.35 | 0.85 | PSM | BM | SB1 | |
| J060931.9+241038 | 10.5 ± 3.2 | 3.986 | 14.41 | 0.71 | PSM | BLM | SB2 | |
| J060923.5+243115 | 16.9 ± 4.3 | 1.288 | 15.32 | 0.96 | PSM | SM | ||
| J060801.8+242645 | 13.1 ± 4.6 | 0.952 | 15.90 | 0.84 | PSM | |||
Notes.The X-ray fluxes in the 0.5−4.5 keV band have been extracted from the XMM-Newton Serendipitous Source Catalog. The rotation periods, extinction-corrected V0 magnitudes, and reddening-corrected (B − V)0 and (V − I)0 colour indices are from M09. The last columns of the table provide indications (see notes at the bottom of the table) about the photometric and spectroscopic membership of each star to M 35 according to M09, and their singularity or binarity according to Geller et al. (2010). (1) PM: photometric member; PNM: photometric non-member; PSM: photometric and spectroscopic member (from M09). (2) BM: binary member; BN: binary non-member; BLM: binary likely member; SM: single member star; SN: single non-member; U: unknown membership status (from Geller et al. 2010).
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