The microwave background and (m, Z) relations in a tilted cosmological model

Details The microwave background and (m, Z) relations in a tilted cosmological model The microwave background and (m, Z) relations in a tilted cosmological model

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..193m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 1, May 1985, p. 193-202.

Astronomy and Astrophysics

Astrophysics

5

Background Radiation, Cosmology, Relic Radiation, Space Temperature, Anisotropy, Dipole Moments, Fluid Flow, Geodesic Lines, Quadrupoles, Red Shift, Space-Time Functions, Temperature Profiles

Scientific paper

The structure of the cosmic microwave background temperature is studied in the context of a Bianchi type-V tilted cosmological model. First integrals of the equations for the null geodesics are found by use of the symmetries of the model, enabling the celestial temperature distribution to be found. The quadrupole and dipole moments are calculated for some models, suggesting that the observed anisotropy in the cosmic microwave background can be understood in the context of a Bianchi type-V model of the Universe. The apparent magnitude-redshift relations are also calculated for these models.

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