Table 3: Unabsorbed fluxes, luminosities, and the conversion efficiencies of PSR B1929+10 and the nebular components in 0.5-10 keV.
Component $f_{\rm X}$ $L_{\rm X}$a $L_{\rm X}/\dot{E}$
  erg s-1 cm-2 erg s-1  
PSR B1929+10 $2.5\times 10^{-13}$ $3.9\times 10^{30}$ $1.0\times 10^{-3}$
Trail-like featureb $5.3\times 10^{-14}$ $8.3\times 10^{29}$ $2.1\times 10^{-4}$
Arc-like feature $1.7\times 10^{-14}$ $2.7\times 10^{29}$ $6.9\times 10^{-5}$
a Luminosities are calculated at the assumed pulsar distance of 361 pc.
b Adopted from Becker et al. (2006).

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