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Table 2.
Model parameterization of Cygnus X-1 that fits the observational data.
Accretion Disk-Corona | |||
---|---|---|---|
Parameter | High/Soft | Hard/Low | Description |
Rin/RISCO | 1 | 20 | inner disk boundary |
ṁ | 0.007 | 0.004 | mass accretion rate |
Rcor/Rg | 20 | 60 | corona radius |
Tcor [keV] | 50 | 150 | corona temperature |
τcor | 0.29 | 0.50 | thermal corona optical depth |
p | 4.9 | 1.8 | corona power-law index |
γmin | 1.8 | 1.7 | minimum energy of nonthermal electrons |
γmax | >20 | >26 | maximum energy of nonthermal electrons |
h | 0.050 | 0.294 | nonthermal/thermal electrons ratio in the corona |
Relativistic Jet | |||
zi [cm] | 3 × 108 | base of the jet | |
zf/zi | 3 | acceleration zone length | |
qrel | 3 × 10−5 | ratio of accelerated to thermal particles | |
ηacc | 0.15 | acceleration efficiency | |
Lp/Le | 0.009 | ratio of the energy carried by hadrons to leptons | |
βjet | 0.92 | bulk velocity | |
ξ [°] | 1.2 | half-opening angle |
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