K-Line Photometry of A Stars

A narrow-band spectrometer, compensated for seeing and transparency variations, has been constructed and used to measure the strength of the calcium K-line (3933.68{AA}) in 146 A-type stars. The observations were made in the spring of 1966 with the No.4 16-inch (40cm) telescope at Kitt Peak National Observatory.

Cone search capability for table II/42/data (Results (table 1 of paper))

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/II/42
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/II/42
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=II/42
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/II/42
Provenance
Creator Henry R.C.
Publisher CDS
Publication Year 2017
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy