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Hydrogen motions in the central region of the Galaxy

Published online by Cambridge University Press:  14 August 2015

B. F. Burke
Affiliation:
Carnegie Institution of Washington, Department of Terrestrial Magnetism
M. A. Tuve
Affiliation:
Carnegie Institution of Washington, Department of Terrestrial Magnetism

Extract

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The 21-cm hydrogen radiation near the galactic plane exhibits strong deviation from circular motion over longitudes within 30° or so of the galactic centre. In order to extend the observations first made by Rougoor and Oort,* the Carnegie multichannel H-line spectrograph was used with our 60-foot radio telescope at Derwood, Maryland, in order to confirm the Leiden work and extend observations to more southern longitudes. Cross-sections extending ±2° in latitude were taken every 2° in longitude from lII=−26°8 to lII=+2°2 and a series of points along the galactic equator were taken every 1° over the same range. Effort has been concentrated on the southern extension of the observations, which agree well with the Leiden observations over the section in common, but which carry the observations nearly 20° farther south in longitude.

Type
Section 1: The Galaxy
Copyright
Copyright © Australian Academy of Science 1964