Non-thermal processes around accreting galactic black holes

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Table 1:

Model parameters.
Parameter	Value
$M_{{\rm BH}}$ : black hole mass [ $M_{\odot}$ ]	10^a
$R_{{\rm c}}$ : corona radius [cm]	$5.2 \times 10^{7}$ ^a,b
$\bf {R_{\rm p}/R_{{\rm c}}}$ : ratio of inner disk to corona radius	0.9^a
D(1+S): Covering fraction of the corona	0.08^a
around thermal disk times the seed
photon correction factor
$T_{\rm e}$ : electron temperature [K]	10⁹
$T_{\rm i}$ : ion temperature [K]	10¹²
$E_{{\rm c}}$ : X-ray spectrum cutoff [keV]	150
$\alpha$ : X-ray spectrum power-law index	1.6
$\eta$ : acceleration efficiency	10^-2
$B_{{\rm c}}$ : magnetic field [G]	$5.7 \times 10^5$
$n_{\rm i},n{\rm e}$ : plasma density [cm^-3]	$6.2 \times 10^{13}$
$A_{{\rm ph}}$ : normalization constant [erg^3/5 cm^-3]	$2.6 \times 10^{12}$
a: hadron-to-lepton energy ratio	1-100
kT: disk characteristic temperature [keV]	0.1
v: advection velocity [c]	0.1

Notes. ^(a) Typical value for Cygnus X-1 in the low-hard state (Poutanen et al. 1997). ^(b) $35~R_{{\rm G}}$ , $R_{{\rm G}}=\frac{GM}{c^{2}}$ .

Source LaTeX | All tables | In the text

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