Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-26T06:30:42.058Z Has data issue: false hasContentIssue false

Origin of protogalactic eddies

Published online by Cambridge University Press:  07 February 2017

A. D. Chernin*
Affiliation:
A. F. Ioffe Physico-Technical Institute Leningrad, USSR

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 highly excited state of the cosmic medium might develop in the isotropic Big Bang starting with weak irrotational perturbations that were likely to be of entropy type. Supersonic matter currents are an indispensable feature of this state. Initial irrotational gas motions become vortical when they become supersonic. One can expect that this may provide a clue in galactic cosmogony (1970, Nature, 226, 440).

Type
V. The Formation of Structure in the Universe
Copyright
Copyright © Reidel 1978