Table 1.
MJD, transition radius, and accretion rate of some of the best fit SED obtained by Marcel et al. (2019) to reproduce the RXTE/PCA observations of the 2010–2011 outburst of GX 339-4.
| MJD | Rtr | Ṁ | L1−1000 Ry | L1−100 keV | Lbol |
|---|---|---|---|---|---|
| (Rg) | (ṀEdd) | (LEdd) | (LEdd) | (LEdd) | |
| 55 208 | 27.1 | 0.63 | 0.019 | 0.014 | 0.043 |
| 55 271 | 23.1 | 1.57 | 0.062 | 0.083 | 0.174 |
| 55 293 | 23.1 | 2.42 | 0.094 | 0.130 | 0.248 |
| 55 294 | 21.6 | 2.42 | 0.099 | 0.132 | 0.249 |
| 55 295 | 9.6 | 2.34 | 0.177 | 0.157 | 0.264 |
| 55 296 | 8.4 | 2.51 | 0.210 | 0.170 | 0.286 |
| 55 297 | 7.2 | 2.80 | 0.261 | 0.194 | 0.324 |
| 55 303 | 5.0 | 2.80 | 0.330 | 0.217 | 0.352 |
| 55 333 | 2.2 | 0.75 | 0.168 | 0.114 | 0.168 |
| 55 334 | 2.0 | 0.70 | 0.166 | 0.115 | 0.166 |
| 55 450 | 2.0 | 0.55 | 0.129 | 0.087 | 0.129 |
| 55 559 | 2.2 | 0.33 | 0.073 | 0.043 | 0.073 |
| 55 565 | 2.5 | 0.34 | 0.070 | 0.040 | 0.070 |
| 55 593 | 3.0 | 0.27 | 0.052 | 0.029 | 0.055 |
| 55 594 | 4.9 | 0.27 | 0.034 | 0.018 | 0.041 |
| 55 601 | 6.6 | 3.33 | 0.033 | 0.019 | 0.044 |
| 55 606 | 15.3 | 0.35 | 0.017 | 0.009 | 0.028 |
| 55 607 | 15.6 | 0.37 | 0.017 | 0.009 | 0.029 |
| 55 617 | 24.2 | 0.15 | 0.005 | 0.003 | 0.008 |
| 55 646 | 40.1 | 0.03 | 0.0006 | 0.0004 | 0.001 |
Notes. We have also reported the corresponding luminosities between 1 and 1000 Rydbergs and between 1 and 100 keV as well as the bolometric luminosity. The Eddington luminosity LEdd = 8.7 × 1038 erg.s−1, assuming a black hole mass of 5.8 M⊙. The distance of GX 339-4 is considered equal to 8 kpc.
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