Table 8
Synoptic table containing the main results concerning the five CVs identified in the present sample of INTEGRAL sources (see Fig. 11).
| Object | Hα | Hβ | He ii λ4686 | R | A V | d | L X | |||
|
|
||||||||||
| EW | Flux | EW | Flux | EW | Flux | mag | (mag) | (pc) | ||
|
|
||||||||||
| Swift J0958.0−4208 | 30.6 ± 1.5 | 34.6 ± 1.7 | 16.1 ± 0.8 | 21.6 ± 1.1 | 19.6 ± 1.0 | 26.5 ± 1.3 | 15.5a | ~0 | ~200 | 2.2 (2–10; X) |
| 6.7 (17–60; I) | ||||||||||
| 4.0 (15–150; B) | ||||||||||
| 4.4 (14–195; B) | ||||||||||
| IGR J14257−6117 | 75 ± 5 | 8.4 ± 0.6 | 18 ± 3 | 1.4 ± 0.2 | 16 ± 2 | 1.19 ± 0.18 | 17.2 | ~2.3 | 1000b | 53 (2–10; X) |
| 87 (17–60; I) | ||||||||||
| 130 (14–195; B) | ||||||||||
| IGR J17014−4306 | 11.1 ± 0.6 | 16.4 ± 0.8 | 13.2 ± 1.3 | 16.1 ± 1.6 | 10.4 ± 1.6 | 11.9 ± 1.8 | 15.1 | ~0 | ~170 | 0.90 (0.2–12; N) |
| 2.5 (17–60; I) | ||||||||||
| 3.0 (15–150; B) | ||||||||||
| 5.5 (14–195; B) | ||||||||||
| IGR J18151−1052 | 29 ± 2 | 0.89 ± 0.06 | 12 ± 4 | 0.10 ± 0.03 | <10 | <0.08 | ≈18c | ~3.6 | 1000b | 48 (2–10; X) |
| 110 (17–60; I) | ||||||||||
| 110 (15–150; B) | ||||||||||
| AX J1832.3−0840 | 50 ± 5 | 1.50 ± 0.15 | 43 ± 9 | 0.37 ± 0.07 | 36 ± 12 | 0.15 ± 0.05 | 19.6c | ~1.1 | 1000b | 110 (0.2–12; N) |
| 130 (0.7–10; A) | ||||||||||
| 84 (2–10; N) | ||||||||||
| 74 (17–60; I) | ||||||||||
| 45 (20–100; I) | ||||||||||
Notes.EWs are expressed in Å, line fluxes are in units of 10-15 erg cm-2 s-1, X-ray luminosities are in units of 1031 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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