Teff for B, A and F main sequence stars Virtual Observatory Resource

Authors

1. SOKOLOV N.A.

Published by

CDS

Abstract

A method of determination of the effective temperature of B, A and F main sequence stars is proposed, using the slope of the continuum between 3200A and 3600A. We have determined the Balmer jump and the effective temperatures for 235 main sequence stars.

Keywords

1. spectrophotometry
2. ultraviolet-astronomy
3. b-stars
4. effective-temperature

Bibliographic source Bibcode

1995A&AS..110..553S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/110/553

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+AS/110/553

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/110/553
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/110/553
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/110/553

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