Table 1: Derived columns, areal coverages, and radial velocities (km s-1) inferred from UV resonance lines.

N V lines		 ($\xi = 75$ km s-1)$\colon$              
$T_{\rm disk}$ Col. density   Fractional Area Vel. Vel. $\tau_{\rm line}$ $\tau_{\rm line}$
  (Abs)    (Emis) (Abs) (Emis) (Abs) (Emis) (Abs) (Emis)
34 000 $1.5\times10^{19}$ - 1.0 0.0 0 - 0.3 -
34 000 $1.5\times10^{19}$ $5\times10^{18}$ 0.4 0.4: 0 +75 0.3 0.1

28 000

 $3\times10^{21}$ - 1.0 0.0 0 - 0.6 -
28 000 $3\times10^{21}$ $3\times10^{21}$ 0.4 0.4: 0 +50 0.6 0.6

C IV lines

 ($\xi = 90$ km s-1)$\colon$              
$T_{\rm disk}$ Col. density   Fractional Area Vel. Vel. $\tau_{\rm line}$ $\tau_{\rm line}$
  (Abs)    (Emis) (Abs) (Emis) (Abs) (Emis) (Abs) (Emis)

24 000		 $3\times10^{21}$ - 1.0 0.2 0 - 15 -
24 000 $3\times10^{21}$ $3\times10^{21}$ 0.4 0.8 0 +125 5 5

20 000

 $3.5\times10^{19}$ - 1.0 0.0 0 - 40 -
20 000 $1.7\times10^{17}$ $1.7\times10^{17}$ 0.4 1.0 0 +125 0.2 0.2
Si IV $\lambda $1403 ($\xi = 75$)$\colon$              
$T_{\rm disk}$ Col. density   Fractional Area Vel. Vel. $\tau_{\rm line}$ $\tau_{\rm line}$
  (Abs)    (Emis) (Abs) (Emis) (Abs) (Emis) (Abs) (Emis)
22 000 $5\times10^{18}$ - 1.0 0.0 0 - 2 -
22 000 $5\times10^{18}$ $5\times10^{18}$ 1.0 2.0 +25 +50 2 2

18 000

 $3\times10^{18}$ - 1.0 0.0 0 - 1.5 -
18 000 $3\times10^{18}$ $3\times10^{18}$ 1.0 6.5 +25 +50 1.5 1.5


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