EINSTEIN A COEFFICIENTS AND OSCILLATOR STRENGTHS FOR THE A 2 Π- X 2 Σ + (RED) AND B 2 Σ + -X 2 Σ + (VIOLET) SYSTEMS AND ROVIBRATIONAL TRANSITIONS IN THE X 2 Σ + STATE OF CN-Reference-Cited by-同舟云学术

EINSTEIN A COEFFICIENTS AND OSCILLATOR STRENGTHS FOR THE A 2 Π- X 2 Σ + (RED) AND B 2 Σ + -X 2 Σ + (VIOLET) SYSTEMS AND ROVIBRATIONAL TRANSITIONS IN THE X 2 Σ + STATE OF CN

Published:2014-01-23 Issue:2 Volume:210 Page:23
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Brooke James S. A.,Ram Ram S.,Western Colin M.,Li Gang,Schwenke David W.,Bernath Peter F.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/0067-0049/210/2/23/pdf

Reference90 articles.

1. ATMOSPHERIC COMPOSITION OF WEAKGBAND STARS: CNO AND Li ABUNDANCES

2. The Circumstellar Shell of the Post–Asymptotic Giant Branch Star HD 56126: The12CN/13CN Isotope Ratio and Fractionation

3. Theoretical study of the dissociation energy and the red and violet band systems of CN

4. First observations of CN (2-1), HCO+ (3-2) and C2H (3-2) emission lines in the Perseus cluster: constraints on heating mechanisms in the cluster gas

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