Abstract
On the basis of the observed satisfactory agreement between recent experimental and calculated Stark width values with our earlier predicted ones along the beryllium isoelectronic sequence (BeI, BII, CIII, NIV, OV FVI, NeVII,..) new Stark width values have been predicted for high ionized emitters (NaVIII, MgIX, AlX, SiXI and PXII) in the 3s-3p transition interesting for astrophysical investigations.
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