Cosmological proper motion

Details Cosmological proper motion Cosmological proper motion

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..845k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 63, Sept.-Oct. 1986, p. 845-849. In Russian.

Mathematics

Logic

5

Celestial Mechanics, Extragalactic Radio Sources, Relic Radiation, Solar System, Astronomical Models, Brightness Temperature, Cosmology, Radio Interferometers

Scientific paper

It is shown that the motion of the solar system relative to the relic radioemission background allows the prediction of the magnitude of the regular proper motion of all extragalactic objects. The mass measurement of this effect through the use of space radiointerferometers will also permit the determination of the basic parameters of a cosmological model. The most appropriate objects for observations are extragalactic sources of synchrotron radiation and H2O masers, the optimal observation range being 1.35-6 cm.

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