Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-29T11:47:44.650Z Has data issue: false hasContentIssue false
  • English
  • Français

Atomic hydrogen survey near the galactic plane

Published online by Cambridge University Press:  14 August 2015

B. F. Burke ,
E. T. Ecklund ,
J. W. Firor ,
H. E. Tatel  and
M. A. Tuve
B. F. Burke
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, Washington, D.C., U.S.A.
E. T. Ecklund
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, Washington, D.C., U.S.A.
J. W. Firor
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, Washington, D.C., U.S.A.
H. E. Tatel
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, Washington, D.C., U.S.A.
M. A. Tuve
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution, Washington, D.C., U.S.A.

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.

Using an 8-meter Würzburg parabola on an equatorial mount in Washington, D. C., we have completed about half of the necessary observations and reductions for a survey of the 1420-Mc/s hydrogen emission for all sky areas near the galactic plane which are visible here.

Type
Part III: Galactic and Extragalactic Radio Sources
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 374 - 389
Copyright
Copyright © Stanford University Press 1959