Structure of the Galaxy and the Sense of Rotation of Spiral Nebulæ

Details Structure of the Galaxy and the Sense of Rotation of Spiral Nebulæ Structure of the Galaxy and the Sense of Rotation of Spiral Nebulæ

Mar 1950

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1950natur.165..487b&link_type=abstract

Nature, Volume 165, Issue 4195, pp. 487-488 (1950).

Computer Science

2

Scientific paper

WE have recently completed a survey of galactic noise over the southern
skies at a frequency of 100 Mc./s.1. This, in conjunction
with previous surveys by Hey, Parsons and Pnillips2 (64
Mc./s.) and Reber3 (160 Mc./s.), has been used to provide
information on the distribution of material in our galaxy.

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