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| MJD | 
|
Si III] | C III] | N III] | O III] | N IV] | O IV] | Si IV | C IV | N V | He II |
| IP [eV] | 16.3 | 24.4 | 29.6 | 35.1 | 47.4 | 54.1 | 33.5 | 47.5 | 77.5 | 54.4 | |
| AX Per | |||||||||||
| 44 156 | 0.000 | -123 | -121 | -120(2) | -124(2) | -106 | -105(2) | -113 | |||
| 45 642 | 0.183 | -137 | -131 | -134(1) | -136(5) | -135 | -135 | -107(4) | -111(1) | -137 | |
| 48 226 | 0.979 | -111 | -110 | -116(2) | -111(2) | -111 | -104(2) | -103(2) | -113 | ||
| SY Mus | |||||||||||
| 44 767 | 0.340 | 7 | 15 | 7 | 9(1) | 8 | 13 | 19(1) | 22(2) | 16(3) | 3 |
| 45 020 | 0.746 | -6 | -10 | 20(1) | 2 | ||||||
| 48 451 | 0.240 | 9 | 10 | 2(1) | 7 | 23(2) | -6 | ||||
| 48 473 | 0.275 | 14 | 19 | 14 | 13(1) | 10 | 26 | 27(1) | 28 | 3 | |
| 48 629 | 0.525 | 16 | 16 | 16(1) | 16(1) | 13 | 21(1) | 23(1) | 22(4) | 12 | |
| 48 623 | 0.675 | 11 | 14 | 9 | 11(1) | 13 | 18(2) | 23(1) | 21(1) | 8 | |
| 50 187 | 0.018 | 0 | 5 | -15 | -2 | -5 | 23(1) | -3 | |||
| RW Hya | |||||||||||
| 44118 | 0.437 | 10 | 11 | 3 | 2(1) | -8 | -3(2) | 17(1) | 26(3) | 19(1) | -26 |
| 44 256 | 0.809 | 7 | 6 | 7 | 6(2) | 8 | 32(2) | 24 | 36(1) | 32(7) | 34 |
| 44 692 | 0.987 | 14 | 23 | 17 | 18(1) | 24 | 47(1) | 45(3) | 55 | ||
| 52 012* | 0.749 | 11.9(0.5) | 17.7 | 35.3(0.1) | 29.0(1.0) | 40.0(1.2) | 46.5 (0.4) | 40.4 | |||
| 52 016* | 0.760 | 8.7(0.3) | 16.1 | 34.0(0.5) | 29.4(0.4) | 38.0(1.3) | 48.1(0.4) | 39.0 | |||
| 52 020* | 0.771 | 9.5(0.8) | 17.1 | 35.4(0.5) | 30.3(0.2) | 39.0(0.9) | 50.1(0.5) | 40.2 | |||
| 52 024* | 0.782 | 11.9(1.1) | 20.0 | 39.2(0.5) | 33.9(0.5) | 42.6(0.8) | 52.9(0.9) | 43.7 | |||
| 52 028* | 0.793 | 10.3(1.3) | 19.8 | 39.9(0.5) | 32.9(0.6) | 42.1(0.5) | 53.3(1.3) | 44.3 | |||
| 52 032* | 0.803 | 12.8(1.4) | 23.2 | 43.5(0.6) | 34.4(0.7) | 45.3(0.4) | 57.6(1.5) | 48.1 | |||
| 52 036* | 0.814 | 13.8(1.3) | 25.0 | 45.0(0.9) | 36.6(0.4) | 46.4(0.2) | 61.9(0.9) | 49.7 | |||
| 52 040* | 0.825 | 14.7(1.5) | 26.2 | 46.0(0.7) | 34.6(1.4) | 46.7(0.2) | 63.3(1.1) | 51.0 | |||
Notes. For saturated lines the radial velocities (itallic) were obtained by fitting their wings. 1-
errors of the mean values are in brackets.
(*) - HST STIS spectra.
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