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Cited by 261

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Generation of microwave background fluctuations from nonlinear perturbations at the ERA of galaxy formation

Ostriker, J. P., Vishniac, E. T.·1986·The Astrophysical Journal

Abstract

The production of temperature distortions of the microwave background by primordial galaxy formation is investigated theoretically. The temperature anisotropies induced by the presence of hot ionized gas during the formation of structure are roughly approximated and found to be greater than the initial anisotropies predicted by hierarchical models, and close to the present upper limit (delta (T/T = about 0.00001 at angular scale 1 arcmin) for standard cold-dark-matter models with Omega(0) = Omega(b) = H/(100 km/s) = 1. It is suggested that sensitive small-scale microwave-fluctuation measurements can impose significant constraints on models of primordial galaxy formation.

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Metadata

Authors
Ostriker, J. P., & Vishniac, E. T.
Venue
The Astrophysical Journal
Published
1986-07
Volume
306
Pages
L51
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1987801517
Cited by
261
References
0
FWCI
8.49
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Generation of microwave background fluctuations from nonlinear perturbations at the ERA of galaxy formation. https://app.cochat.ai/papers/10.1086/184704
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Ostriker, J. P., & Vishniac, E. T. (1986). Generation of microwave background fluctuations from nonlinear perturbations at the ERA of galaxy formation. The Astrophysical Journal. https://doi.org/10.1086/184704

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