Neutron capture elements in stars: neodymium Virtual Observatory Resource

Authors

1. Mashonkina L.I.
2. Kamaeva L.A.
3. Samotoev V.A.
4. Sakhibullin N.A.

Published by

CDS

Abstract

We have derived the LTE neodymium abundances in 60 cool stars with [Fe/H] from 0.25 to -1.71 by applying a synthetic-spectrum analysis to spectroscopic observations of NdII lines with a resolution of {lambda}/{Delta}{lambda}~60000 and signal-to noise ratios of 100-200.

Keywords

1. dwarf-stars
2. spectroscopy
3. chemical-abundances

Bibliographic source Bibcode

2004AZh....81..209M

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/81/209

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ivo://CDS.VizieR/J/AZh/81/209

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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/81/209

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http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/81/209/table1?