Bar-induced strengths in spiral galaxies

DOI

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.

Cone search capability for table J/MNRAS/355/1251/table2 (Structural parameters from 2D decompositions)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73551251
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/355/1251
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/355/1251
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/355/1251
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/355/1251
Provenance
Creator Laurikainen E.; Salo H.; Buta R.; Vasylyev S.
Publisher CDS
Publication Year 2006
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics