Rotationally resolved gas-phase spectrum of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si7.svg"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="normal">A</mml:mi><mml:mo stretchy="false">∼</mml:mo></mml:mover></mml:mrow></mml:math> 2Σ+–<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si8.svg"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="normal">X</mml:mi><mml:mo stretchy="false">∼</mml:mo></mml:mover></mml:mrow></mml:math> 2Π3/2 electronic transition for the cyanogen halide radical cation ICN+-Reference-Cited by-同舟云学术

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Rotationally resolved gas-phase spectrum of the A∼ 2Σ+–X∼ 2Π3/2 electronic transition for the cyanogen halide radical cation ICN+

Published:2022-07 Issue: Volume:388 Page:111675
ISSN:0022-2852
Container-title:Journal of Molecular Spectroscopy
language:en
Short-container-title:Journal of Molecular Spectroscopy

Author:

Araki Mitsunori,Ito Takumi,Hoshino Shoma,Tsukiyama Koichi

Publisher

Elsevier BV

Subject

Physical and Theoretical Chemistry,Spectroscopy,Atomic and Molecular Physics, and Optics

Reference29 articles.

1. The diffuse interstellar bands;Herbig;Annu. Rev. Astron. Astrophys.,1995

2. J. Cami, N.L.J. Cox, The diffuse interstellar bands, in: Proc. Int. Astron. Union, IAU Symp., Cambridge University Press, Noordwijkerhout, The Netherlands, 2014.

3. Further study of the sodium lines in class B stars;Heger;Lick Obs. Bull.,1922

4. On the discovery of the diffuse interstellar;McCall;bands,2013

5. Laboratory confirmation of C60+ as the carrier of two diffuse interstellar bands;Campbell;Nature,2015

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