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Large Scale Coherent Star-Formation in NGC 4321
Published online by Cambridge University Press: 03 August 2017
Abstract
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We apply a newly devised quantitative technique to infer the relative arm/interarm star formation efficiency ratio in NGC 4321, revealing a complex but clearly defined density wave structure pattern.
- Type
- III- Observations of Spiral Structure
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- Copyright © Kluwer 1991
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