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Extended rotation curves of high-luminosity spiral galaxies. IV - Systematic dynamical properties, SA through SC
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1978
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Galaxy FormationPhotometrySystematic Dynamical PropertiesEngineeringAstronomical Coordinate SystemPhysicsNatural SciencesAccurate Rotation CurvesAstrodynamicsAstrophysical SimulationVaucouleurs RadiiLarge Scale StructureRotation CurvesHigh-luminosity Spiral GalaxiesAstrophysics
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.