Effective temperatures of Ap stars Virtual Observatory Resource

Authors

1. Sokolov N.A.

Published by

CDS

Abstract

A new method of determination of the effective temperatures of Ap stars is proposed. The method is based on the fact that the slopes of the energy distribution in the Balmer continuum near the Balmer jump for "normal" main sequence stars and Ap stars with the same effective temperature are identical. The effective temperature calibration is based on a sample of main sequence stars with well known temperatures (Sokolov, 1995, Cat. <J/A+AS/110/553>).

Keywords

1. peculiar-variable-stars
2. effective-temperature

Bibliographic source Bibcode

1998A&AS..130..215S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/130/215

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+AS/130/215

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/130/215
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/130/215
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/130/215

IVOA Table Access TAP

https://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).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+AS/130/215/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+AS/130/215/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+AS/130/215/table1?