Extended rotation curves of high-luminosity spiral galaxies. IV - Systematic dynamical properties, SA through SC
The Astrophysical JournalPublished 1 November 1978
V. C. Rubin, N. Thonnard, Jr. Ford W. K.
Citations530
SJR quartileQ1
SJR score2.04
SNIP1.25
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Abstract
For a sample of 10 high-luminosity spiral galaxies, Sa through Sc, we have obtained accurate rotation curves which extend to about 80% of the de Vaucouleurs radii.
Keywords
Physics and Astronomy