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Table 3
Absorbing column density NH, photon index Γ and normalisation factor PL of absorbing power-laws describing the Chandra spectra (see Fig. 4 and text).
| NH | Γ | PL | C (nbins) |
| 10 cm | 10 ph cm s keV | ||
|
|
|||
| pulsar | |||
|
|
|
245 (649) |
| pulsar+PWN | |||
|
|
|
448 (649) |
| south-east tail of the PWN | |||
|
|
|
267 (649) |
Notes. Errors correspond to ΔC = 1.
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