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• Spectral line broadening i t h i l l i t h i l l in astrophysical plasmas

• Spectral line broadening i t h i l l i t h i l l in astrophysical plasmas

• Spectral line broadening i t h i l l i t h i l l in astrophysical plasmas

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Here v barr is the average relative velocity ofcollid<strong>in</strong>g atoms and N zero perturber density.•

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