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Radial velocities of neutral hydrogen in the anticenter region of the Galaxy
Published online by Cambridge University Press: 14 August 2015
Abstract
An observational material of 21-cm H I emission-line profiles is investigated by a statistical method to derive the kinematical properties of the interstellar gas in the region of the galactic anticenter. A description of the method used as well as the results obtained, concerning deviations from a circular rotation, are given.
- Type
- Part II/Observations of Spiral Structure in Our Galaxy
- Information
- Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 164 - 168
- Copyright
- Copyright © Reidel 1970
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