Bibcode
Betancort-Rijo, J. E.
Referencia bibliográfica
Astronomy and Astrophysics, v.299, p.635
Advertised on:
7
1995
Revista
Número de citas
1
Número de citas referidas
1
Descripción
The models for galaxy clustering in which galaxies are identified with
peaks on the mass density field smoothed on an appropriate scale are
plagued by some difficulties. We discuss them here, propose an
alternative model that avoids them and compute the correlation functions
implied by it. This model has been developed within the context of the
recently developed theory for structures in random Gaussian fields.