Neutron capture elements in stars: neodymium

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.

Cone search capability for table J/AZh/81/209/table1 (Stellar parameters of the selected sample and the final [Nd/Fe] ratios)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AZh/81/209
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/81/209
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/81/209
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AZh/81/209
Provenance
Creator Mashonkina L.I.; Kamaeva L.A.; Samotoev V.A.; Sakhibullin N.A.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy