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Published:2006-07-10 Issue:2 Volume:645 Page:1560-1567
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Liu Xianming,Shemansky Donald E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference63 articles.

1. Theoretical calculations of excited rovibrational levels of HD. Term values and transition probabilities of VUV electronic bands

2. High resolution EUV emission spectroscopy of the and 4 levels by electron impact

3. Medium-resolution studies of extreme ultraviolet emission fromN2by electron impact: Vibrational perturbations and cross sections of thec4’Σu+1and b’Σu+1states

4. Ab initio and configuration interaction calculations of optical oscillator strengths for the N2molecule

Cited by 12 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Opacities of <inline-formula><tex-math id="Z-20220715033133-1">\begin{document}${ X}^1\Sigma^+_{\rm g}, a'{}^1\Sigma^-_{\rm u}, a{}^1\Pi_{\rm g} \text{ and } { b}^1\Pi_{\rm u}$\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="14-20220043_Z-20220715033133-1.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="14-20220043_Z-20220715033133-1.png"/></alternatives></inline-formula> electronic states for nitrogen molecule;Acta Physica Sinica;2022

2. SPECTRA, EMISSION YIELDS, CROSS SECTIONS, AND KINETIC ENERGY DISTRIBUTIONS OF HYDROGEN ATOMS FROM H2${X}^{1}{{\rm{\Sigma }}}_{g}^{+}$–${d}^{3}{{\rm{\Pi }}}_{u}$ EXCITATION BY ELECTRON IMPACT;The Astrophysical Journal;2016-02-12

3. ABSORPTION OSCILLATOR STRENGTHS FOR THE c(4)(' 1)Sigma(+)(u)(3,4,6)-X-1 Sigma(+)(g)(nu ''), b(' 1)Sigma(+)(u)(10,13,20)-X-1 Sigma(+)(g)(nu ''), AND c(5)(' 1)Sigma(+)(u)(1)-X-1 Sigma(+)(g)(nu '') PROGRESSIONS IN N-2;ASTROPHYS J;2016

4. 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;The Astrophysical Journal;2016-01-05

5. THE HIGH-RESOLUTION EXTREME-ULTRAVIOLET SPECTRUM OF N 2 BY ELECTRON IMPACT;The Astrophysical Journal Supplement Series;2014-04-02