|journal=Monthly Notices of the Royal Astronomical Society
|journal=Monthly Notices of the Royal Astronomical Society
|volume=460
|volume=460
−
|issue=4|page=4038-4062|date=2016
+
|issue=4|pages=4038–4062|date=2016
|doi=10.1093/mnras/stw1243
|doi=10.1093/mnras/stw1243
|bibcode=2016MNRAS.460.4038E
|bibcode=2016MNRAS.460.4038E
Line 42:
Line 42:
|journal=Monthly Notices of the Royal Astronomical Society
|journal=Monthly Notices of the Royal Astronomical Society
|volume=456
|volume=456
−
|issue=4|page=4305-4314|date=2016
+
|issue=4|pages=4305–4314|date=2016
|doi=10.1093/mnras/stv2819
|doi=10.1093/mnras/stv2819
|bibcode=2016MNRAS.456.4305T
|bibcode=2016MNRAS.456.4305T
|ref=harv
|ref=harv
−
}} {{arXiv|1310.2801}}</ref> The [[electron]] [[density]] has been found to be around 0.4 cm<sup>-3</sup> for this plasma.<ref name=xray/> Inhomogeneities in the [[nitrogen]] abundance and temperature distribution have also been detected.
+
}} {{arXiv|1310.2801}}</ref> The [[electron]] [[density]] has been found to be around 0.4 cm<sup>−3</sup> for this plasma.<ref name=xray/> Inhomogeneities in the [[nitrogen]] abundance and temperature distribution have also been detected.