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HI and HII in Nearby Spiral Galaxies
Published online by Cambridge University Press: 03 August 2017
Extract
Spiral arm properties varies widely from one galaxy to another. For this reason detailed observational studies of galaxies with different morphologies are critical for the understanding of the role, if any, of the spiral arms, in the formation of the complexes of HI clouds, molecular clouds and ultimately for the formation of the massive stars.
- Type
- VI- Other Gaseous Components
- Information
- Copyright
- Copyright © Kluwer 1991