OI and FeII equivalent widths in metal-poor stars

DOI

The table gives equivalent widths (in m{AA}) of OI and FeII lines for 35 metal-poor main sequence and subgiant stars as measured from high resolution, high S/N spectra observed with the ESO VLT/UVES spectrograph, during three observing runs: April 8-12, 2000, July 22-24, 2000, and April 10-12, 2001.

Cone search capability for table J/A+A/390/235/stars (Star positions and magnitudes (from Simbad))

Identifier
DOI http://doi.org/10.26093/cds/vizier.33900235
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/390/235
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/390/235
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/390/235
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/390/235
Provenance
Creator Nissen P.E.; Primas F.; Asplund M. Lambert D.L.
Publisher CDS
Publication Year 2002
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