Bibcode
DOI
Watson, R. A.; Gutierrez de La Cruz, C. M.; Davies, R. D.; Lasenby, A. N.; Rebolo, R.; Beckman, J. E.; Hancock, S.
Referencia bibliográfica
Nature (ISSN 0028-0836), vol. 357, no. 6380, June 25, 1992, p. 660-665.
Fecha de publicación:
6
1992
Número de citas
60
Número de citas referidas
51
Descripción
Galaxy formation by gravitational instability implies the presence of
temperature fluctuations in the cosmic microwave background. New
observations at 10.45 and 14.9 GHz from the Observatorio del Teide in
Tenerife on angular scales of several degrees reveal structure of
galactic origin at the lower frequency, while at the upper frequency the
magnitude of fluctuations of cosmological origin must be less than 1.8 x
10 exp -5 on a scale of 5 deg. This strongly constrains models of galaxy
formation, and is compatible with the recently announced discovery by
the COBE satellite of fluctuations on larger angular scales.