Bar-induced strengths in spiral galaxies (Laurikainen+, 2004)

Details Bar-induced strengths in spiral galaxies (Laurikainen+, 2004) Bar-induced strengths in spiral galaxies (Laurikainen+, 2004)

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..73551251l&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/355/1251. Originally published in: 2004MNRAS.355.1251L

Physics

Galaxies: Nearby, Morphology

Scientific paper

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.
(1 data file).

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