Table 8
Synoptic table containing the main results for the active stars (see Fig. 8) identified in the present sample of INTEGRAL sources.
| Object | Hα | R | d | LX | |
|
|
|||||
| EW | Flux | mag | (pc) | ||
|
|
|||||
| IGR J18371+2634(#1) | 0.59 ± 0.12 | 13 ± 3 | 12.5 | 530 | 0.0057 (0.1–2.4; R) |
| 0.0044 (2–10; X) | |||||
| 0.47 (20–40; I) | |||||
| < 0.47 (40–100; I) | |||||
| IGR J23130+8608 | 0.74 ± 0.07 | 2.1 ± 0.2 | 14.7 | 1500 | 0.019 (2–10; X) |
| 3.8 (20–40; I) | |||||
| <4.6 (40–100; I) | |||||
Notes. EWs are expressed in Å, line fluxes are in units of 10-15 erg cm-2 s-1, whereas X-ray luminosities are in units of 1033 erg s-1 and the reference band (between round brackets) is expressed in keV. In the last column, the upper-case letter indicates the satellite and/or the instrument with which the corresponding X-ray flux measurement was obtained (see text).
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