Theoretical isochrones in the case of stellar evolution with variable G /Brans-Dicke cosmological theory/

Details Theoretical isochrones in the case of stellar evolution with variable G /Brans-Dicke cosmological theory/ Theoretical isochrones in the case of stellar evolution with variable G /Brans-Dicke cosmological theory/

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..817l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, June 1979, p. 817-821.

Mathematics

Logic

Astronomical Maps, Cosmology, Gravitational Constant, Stellar Evolution, Astronomical Models, Galactic Clusters, Hertzsprung-Russell Diagram, Lines (Geometry), Open Clusters, Stellar Mass

Scientific paper

Theoretical isochrones for three and five billion years of age appropriate to open clusters have been computed assuming the Brans-Dicke cosmological theory. These are compared with the standard isochrones and the ones obtained by other investigators under various assumptions for the variation of the gravitational constant. The comparison shows that stellar evolution is not able to test the correctness of the Brans-Dicke cosmological theory.

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