X-ray emitting structures in the Vela SNR: ejecta anisotropies and progenitor stellar wind residuals

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Table 5

ROSAT filament best-fit.

Parameter	Ext_fil
N_H (10²² cm⁻²)
kT (keV)
O/O_⊙
Ne/Ne_⊙	<1.5
n²l (10¹⁸ cm⁻⁵)
χ²∕d.o.f.	93.15/94

Notes. The abundance of O was frozen to the best-fit parameter in order to reduce the uncertainty of the kT parameter. The abundance of O was determined by freezing Ne abundance. Errors are at a 90% confidence level.

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