The 15N-enrichment in dark clouds and Solar System objects
The 15N-enrichment in dark clouds and Solar System objects
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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
The line intensities of the fundamental rotational transitions of H13CN and HC15N were observed towards two prestellar cores, L183 and L1544, and lead to molecular isotopic ratios 140 6 14N/15N 6 250 and 140 6 14N/15N 6 360, respectively. The range of values reflect genuine spatial variations within the cores. A comprehensive analysis of the availa...
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Full title
The 15N-enrichment in dark clouds and Solar System objects
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TN_cdi_proquest_journals_2083064318
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2083064318
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1302.6318
