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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

L. Velden
L. Velden*
Affiliation:
Astronomische Institute der Universität Bonn, Bonn, Germany

Abstract

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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 

References

Grahl, B. H., Hachenberg, O., and Mebold, U.: 1968, Beiträge zur Radioastronomie 1, 3.Google Scholar
Schmidt, M.: 1965, Stars and Stellar Systems 5, 513.Google Scholar
Schwartz, R.: 1967, Forschungsberichte des Landes Nordrhein-Westfalen, Nr. 1844, Westdeutscher Verlag Köln-Opladen.Google Scholar
Velden, L.: 1970, ‘Atlas of 21-cm Line Profiles of the Outer Part of the Galaxy in the Region of the Galactic Anticenter’, Beiträge zur Radioastronomie, in preparation.Google Scholar