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Correlation Functions, Microwave Background, and Pancakes

Published online by Cambridge University Press:  04 August 2017

S. A. Bonometto  and
F. Lucchin
S. A. Bonometto
Affiliation:
Istituto di Fisica “G. Galilei,” Via Marzolo, 8, Padova, Italy I.N.F.N., Sez. di Padova
F. Lucchin
Affiliation:
Istituto di Fisica “G. Galilei,” Via Marzolo, 8, Padova, Italy

Extract

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The isothermal theories of galaxy formation encounter serious difficulties in accounting for the existence of large voids (see, e.g., Aarseth and Saslow 1982). The alternative picture of adiabatic fluctuations and pancake collapse (see, e.g., Doroshkevich et al. 1978 and references therein) faces difficulties due to: i) observed correlation functions, and ii) the absence of small-scale fluctuations in the microwave background.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 219 - 221
Copyright
Copyright © Reidel 1983 

References

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Bonometto, S.A., Caldara, A., and Lucchin, F. 1982, submitted to Astron. and Astrophys. Google Scholar
Doroshkevich, A.G., Zeldovich, Ya. B., and Sunyaev, R.A. 1978, Sov. Astron., 22, 523.Google Scholar
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