Table 3: Precession solutions for $\iota = 5$- $8\hbox {$^\circ $ }$.
Parameter Value
$\iota$ $[\hbox{$^\circ$ }]$ 5 6 6.5 7 8
$\Omega _{\rm p}$ $[\hbox{$^\circ$ }]$ 1.3 1.4 1.45 1.5 1.6
$t_{{\rm beam}}$ $[{\rm yr}]$ 220 200 180 165 150
$T_{\rm p}$ $[{\rm yr}]$ 3320 2780 2570 2370 2070
Note: Bold face denotes the best fit solution. $T_{\rm p}$ is calculated
with the best fit value of the Alfvén speed $V_{\rm A} = 0.078~c$.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 The binary black hole model
3 The quasar 3C 345
4 Application of the BBH model
5 Properties of the BBH system in 3C 345
6 Discussion
7 Conclusions
References
List of tables
List of figures