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Large Scale Clustering in the Universe

Published online by Cambridge University Press:  14 August 2015

P. J. E. Peebles

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In 1924 Hubble presented the first generally convincing evidence, from the identification of variable stars, that some of the brightest “spiral nebulae” are galaxies of stars well outside the bounds of our own Galaxy. This led him to reconsider the idea that the faint “spiral nebulae,” which were known to be much more abundant than bright ones, might be similar objects at greater distances.

Type
III. Large Scale Systems
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 217 - 226
Copyright
Copyright © Reidel 1978 

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