K-Line Photometry of A Stars Virtual Observatory Resource

Authors
  1. Henry R.C.
  2. Published by
    CDS
Abstract

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.

Keywords
  1. visible-astronomy
  2. narrow-band-photometry
  3. a-stars
Bibliographic source Bibcode
1969ApJS...18...47H
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/II/42
IVOA Identifier IVOID
ivo://CDS.VizieR/II/42

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=II/42
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=II/42
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=II/42
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/II/42/data?
https://vizier.iucaa.in/viz-bin/conesearch/II/42/data?
http://vizieridia.saao.ac.za/viz-bin/conesearch/II/42/data?

History

2017-01-19T14:08:28Z
Resource record created
2017-01-19T14:08:28Z
Created
2017-11-06T12:23:54Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr