ABSORPTION OSCILLATOR STRENGTHS FOR THE ${{C}_{4}^{\prime }}^{1}{{\rm{\Sigma }}}_{{\Rm{u}}}^{+}$(3, 4, 6)–${X}^{1}{{\rm{\Sigma }}}_{{\Rm{g}}}^{+}(v^{\prime\prime} ),\;$ $B{^{\prime} }^{1}{{\rm{\Sigma }}}_{{\Rm{u}}}^{+}$(10, 13, 20)–${X}^{1}{{\rm{\Sigma }}}_{{\Rm{g}}}^{+}(v^{\prime\prime} ),$ AND ${{C}_{5}^{\prime }}^{1}{{\rm{\Sigma }}}_{{\Rm{u}}}^{+}$(1)–${X}^{1}{{\rm{\Sigma }}}_{{\Rm{g}}}^{+}(v^{\prime\prime} )$ PROGRESSIONS IN N2
Astrophysical Journal - United States
doi 10.3847/0004-637x/816/2/58
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Date
January 5, 2016
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American Astronomical Society