An S2Fluorescence Model for Interpreting High‐Resolution Cometary Spectra. I. Model Description and Initial Results-Reference-Cited by-同舟云学术

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An S2Fluorescence Model for Interpreting High‐Resolution Cometary Spectra. I. Model Description and Initial Results

Published:2003-04-10 Issue:1 Volume:587 Page:464-471
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Reyle Celine,Boice D. C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/587/i=1/a=464/pdf

Reference31 articles.

1. The discovery of S2 in comet IRAS-Araki-Alcock 1983d

2. A’Hearn, M. F., Ohlmacher, J. T. & Schleicher, D. G. 1983b, Univ. Maryland Tech. Rep. TR-AP83-044

3. Franck–Condon factors for the B–X system of S2

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1. Parent Volatile Outgassing Associations in Cometary Nuclei: Synthesizing Rosetta Measurements and Ground-based Observations;The Planetary Science Journal;2024-03-01

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3. Transition properties of the X3Σ–g, A′3Δu, A3Σ+u, B′′3Πu, B3Σ–u, and B′3Πg states of sulphur dimer;Journal of Quantitative Spectroscopy and Radiative Transfer;2020-02

4. Potential energy curves, turning points, Franck–Condon factors and $r$-centroids for the astrophysically interesting $\mbox{S}_{2}$ molecule;Astrophysics and Space Science;2019-10

5. Stability of Sulphur Dimers (S2) in Cometary Ices;The Astrophysical Journal;2017-01-23

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