| TARGET | RASS X-raya,b,c | Log
|
Log ( |
|
HJD | RV | Commentse | ||
| ct rate [ct s-1] | [erg s-1] | [days] | [kms-1] | (+2450000) | [kms-1] | [kms-1] | |||
| Lupus : | |||||||||
| RX J1507.2-3505 |
|
29.99 | -4.09 | 15.0 | 2713.762 | +2.1 | 13.0 | RV = +1.4 | |
| 2718.766 | +2.2 | 13.2 | |||||||
| RX J1507.4-4601 |
|
29.93 | -3.30 | 2718.790 | +6.9 | 21.7 | |||
| RX J1515.7-3331 |
|
30.15 | -3.61 | 2.28 | 25.0 | 2713.860 | +1.1 | 22.3 | |
| 2718.925 | +1.9 | 23.4 | |||||||
| RX J1518.4-3738 |
|
30.26 | -3.36 | 2.98 | 25.0 | 2718.746 | +3.7 | 21.6 | RV = +3.7 |
| RX J1523.4-4055 |
|
29.71 | -3.62 | 4.15 | 9.9 | 2719.769 | +5.6 | 11.7 | RV = +6.8 |
| RX J1524.5-3652 |
|
29.93 | -3.55 | 2.91 | 19.0 | 2713.826 | +4.4 | 16.4 | RV = +4.2 |
| 2719.792 | +4.6 | 17.6 | |||||||
| RX J1525.0-3604 |
|
30.26 | -3.44 | 2718.852 | +4.8 | 23.2 | |||
| RX J1529.6-3546 |
|
30.19 | 2718.879 | +16.4 | 19.3 | SB2 | |||
| 2718.879 | -11.3 | 19.5 | SB2 | ||||||
| RX J1529.7-3628 |
|
29.93 | 2719.715 | +3.2 | 14.5 | ||||
| RX J1546.6-3618 |
|
29.85 | -3.69 | 7.1 | 2713.705 | +7.2 | RV = +2.5 | ||
| 2719.747 | +7.3 | ||||||||
| RX J1547.6-4018 |
|
29.93 | -3.67 | 10.0 | 2713.737 | +3.1 | 11.8 | RV = +2.8 | |
| 2718.916 | +3.2 | 12.9 | |||||||
| RX J1601.1-3320 |
|
30.15 | -3.62 | 3.78 | 21.9 | 2713.799 | +2.3 | 18.8 | RV = +3.0 |
| RX J1605.7-3905 |
|
30.35 | -3.40 | 2713.780 | +2.2 | >50 | |||
| RX J1608.9-3905 | 2718.900 | +9.7 | 30.4 | RV = -0.6 | |||||
| 2718.900 | -25.8 | 24.1 | SB2 | ||||||
| Chamaeleon I |
|||||||||
| RX J0850.1-7554 |
|
30.68 | -3.30 | 45 | 2712.590 | +17.1 | 49.4 | RV = +15.5 | |
| 2718.521 | +35.0 | 26.5 | SB2? | ||||||
| 2718.521 | -0.8 | 23.3 | SB2? | ||||||
| RX J0951.9-7901 |
|
30.68 | -3.54 | 73 | 2712.620 | +39.8 | 49.0 | RV = +12.2 | |
| 2712.620 | -20.3 | 32.6 | SB2? | ||||||
| 2718.533 | +38.1 | 47.2 | SB2? | ||||||
| 2718.533 | -35.1 | 32.3 | SB2? | ||||||
| RX J1112.7-7637 |
|
30.36 | -3.31 | 11 | 2712.694 | +13.6 | 30.7 | RV = +16.0 | |
| 2718.546 | +15.2 | 28.4 | |||||||
| RX J1129.2-7546 | 20 | 2713.628 | +15.9 | 20.8 | RV = +11.4 | ||||
| 2719.528 | +15.5 | 19.9 | |||||||
| RX J1140.3-8321 |
|
30.50 | -3.40 | 13 | 2718.563 | +14.0 | 12.5 | RV = +10.5 | |
| RX J1158.5-7754a |
|
30.93 | -3.45 | 11 | 2713.656 | +10.4 | 15.1 | RV = +13.1 | |
| 2718.614 | +10.1 | 14.7 | |||||||
| RX J1159.7-7601 |
|
30.46 | -3.58 | 10 | 2718.636 | +15.1 | 10.2 | RV = +13.1 | |
| RX J1201.7-7859 |
|
30.76 | -3.96 | 21 | 2712.734 | +12.3 | 22.2 | RV = +10.0 | |
| 2718.678 | +13.6 | 22.2 | RV = +22.3 | ||||||
| RX J1233.5-7523 | 7 | 2712.760 | +14.8 | 7.2 | RV = +14.0 | ||||
| 2718.716 | +16.0 | 6.9 | RV = +15.1 | ||||||
| RX J1239.4-7502 |
|
30.72 | -3.47 | 19 | 2713.675 | +14.5 | 20.2 | RV = +13.1 | |
| 2718.726 | +14.2 | 20.1 | |||||||
| RX J1303.5-7701 | 2712.779 | -121.1 | Early-Type | ||||||
| RX J1307.3-7708 | 2712.794 | -25.3 | |||||||
| Rho Ophiuchus : | |||||||||
| RX J1627.1-2419 | 2712.852 | -2.7 | |||||||
| RX J1625.6-2613 | 2712.886 | -3.5 | 17.0 | ||||||
| CrA SFR : | |||||||||
| CrAPMS 2 |
|
29.93 | -3.79 | 2.79 | 20 | 2713.909 | -0.7 | 20.2 | RV = -2.2,-1.2 |
| 2719.923 | 0.0 | 20.4 | RV = -2.6 | ||||||
| RX J1839.0-3726 | 17.8 | 2719.869 | -1.6 | 9.8 | RV = -4.8 | ||||
| RX J1853.1-3609 |
|
30.28 | -3.68 | 2719.837 | -3.2 | 24.0 | |||
| RX J1917.4-3756 |
|
30.28 | -3.82 | 2713.920 | -0.9 | 28.1 | |||
| 2719.817 | +0.5 | 28.3 | |||||||
| CrAPMS 4SE | <10 | 2719.901 | -1.9 | 9.7 | RV = -2.0 |
|
a The standard RASS conversion factor, for negligible interstellar
absorption, of 6 b These fluxes are lower limits, as it is unlikely that these stars represent a sample of unabsorbed X-ray emitters (see text). c For the ROSAT passband 0.1-2.4 keV. d Distances used for luminosity calculations: Lupus, d= 140 pc (Hughes et al. 1993; Bertout et al. 1999; de Zeeuw et al. 1999); Chamaeleon, d= 160 pc (Bertout et al. 1999; Rebull et al. 2004, and references therein); CrA SFR, d= 120 pc (Morraco & Rydgren 1981; Casey et al. 1998). e Lupus Vsini/Periods/RV data are taken from Wichmann et al. (1998, 1999); Chamaeleon Vsini/RV data are taken from Covino et al. (1997), Cutispoto et al. (2002) & Nordström et al. (2004); CrA SFR Vsini/RVs/Period data are taken from Neuhäuser et al. (2000), Franchini et al. (1992), Walter et al. (1997) & Shevchenko et al. (1995). |