Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-14T05:52:47.478Z Has data issue: false hasContentIssue false
  • English
  • Français

A study of spiral structure for 270° ≤ lII ≤ 310°

Published online by Cambridge University Press:  14 August 2015

S. L. Garzoli
S. L. Garzoli*
Affiliation:
Instituto Argentino de Radioastronomía, Buenos Aires, Argentine

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A survey of the distribution of the intensity of the 21 cm-line of atomic hydrogen in the region with galactic coordinates 270° ≤ lII ≤ 310°, −3° ≤ bII ≤ 2°, was made with the 100-foot radiotelescope and 56-channel receiver of the Radio Astronomy Station of the Instituto Argentino de Radioastronomía and the Department of Terrestrial Magnetism of the Carnegie Institution of Washington. The angular and velocity resolution of the system is 28′ of arc and 2 km s−1.

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. 151 - 153
Copyright
Copyright © Reidel 1970