Bar-induced strengths in spiral galaxies Virtual Observatory Resource

Authors

1. Laurikainen E.
2. Salo H.
3. Buta R.
4. Vasylyev S.

Published by

CDS

Abstract

Bar-induced perturbation strengths are calculated for a well-defined magnitude-limited sample of 180 spiral galaxies, based on the Ohio State University Bright Galaxy Survey. We use a gravitational torque method, the ratio of the maximal tangential force to the mean axisymmetric radial force, as a quantitative measure of the bar strength.

Keywords

1. galaxies
2. galaxy-classification-systems

Bibliographic source Bibcode

2004MNRAS.355.1251L

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/355/1251

IVOA Identifier IVOID

ivo://CDS.VizieR/J/MNRAS/355/1251

Document Object Identifer DOI

doi:10.26093/cds/vizier.73551251

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/355/1251
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/355/1251
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/355/1251

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/J/MNRAS/355/1251/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/355/1251/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/355/1251/table2?