Table 5
Characteristic quantities of the RXTE PCA light curves for Galactic sources presented in Altamirano et al. (2011b; Cols. 4−6) supplemented with HLX and AGNs, and estimations of the mass−α relations and magnetisation of sources (Cols. 7,8).
| Source | ID | P | A | Δ |
|
μ* |
|
|
||||||
| IGR | ν I | 45 s | 2.5 | 0.15 | 6.38 | 0.717 |
| IGR | ρ IA | 30s | 3.5 | 0.3 | 3.52 | 0.634 |
| IGR | ρ IB | 30s | 4 | 0.4 | 3.198 | 0.589 |
| GRS | ν G | 90 s | 4 | 0.1 | 8.31 | 0.763 |
| GRS | ρ GA | 45s | 5 | 0.25 | 3.87 | 0.661 |
| GRS | ρ GB | 40s | 4.5 | 0.4 | 3.77 | 0.583 |
| HLX | – | 400d | 2.5 | 0.14 | 1.88 × 105 | 0.534 |
| AGN* | – | 105y | 100 | 0.1 | 1.6 × 108 | 0.515 |
Notes. IGR = IGR J17091, GRS = GRS1915, HLX = HLX-1, AGN – typical value for the sample of AGNs presented in (Czerny et al. 2009). The OBSIDs of the ligth curves are as follows: νI = 96420−01−05−00 (ν state), ρIA = 96420−01−06−00 (ρ state), ρIB = 96420−01−07−00 (ρ state), νG = 10408−01−40−00 (ν state), ρGA = 20402−01−34−00 (ν state) and ρGB = 93791−01−02−00 (ρ state).
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