Energy distribution of G,K and M stars Virtual Observatory Resource

Authors

1. Knyazeva L.N.
2. Kharitonov A.V.

Published by

CDS

Abstract

A large number of stars from photometrically homogeneous catalogs are used to derive the normal energy distribution for giants of 15 spectral subclasses. To judge the reliability of the results obtained, the mean (B-V)_S_ color indices calculated for a sample of stars with spectrophotometry are compared with the mean (B-V) for a complete sample of stars of a given subclass from the Bright Star (<V/50>) catalog.

Keywords

1. late-type-stars
2. spectral-energy-distribution

Bibliographic source Bibcode

1996AZh....73...67K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/73/67

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AZh/73/67

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/73/67
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/73/67
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/73/67

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).