Radiative lifetimes and cooling functions for astrophysically important molecules
Radiative lifetimes and cooling functions for astrophysically important molecules
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Extensive line lists generated as part of the ExoMol project are used to compute lifetimes for individual rotational, rovibrational and rovibronic excited states, and temperature-dependent cooling functions by summing over all dipole-allowed transitions for the states concerned. Results are presented for SiO, CaH, AlO, ScH, H\(_2\)O and methane. Th...
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Radiative lifetimes and cooling functions for astrophysically important molecules
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TN_cdi_proquest_journals_2078061864
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2078061864
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1601.07997