The evolution of the physical characteristics of theoretical stellar models with variable G /Brans-Dicke cosmological theory/ in isochrones of one, three and five billion years

Details The evolution of the physical characteristics of theoretical stellar models with variable G /Brans-Dicke cosmological theory/ in isochrones of one, three and five billion years The evolution of the physical characteristics of theoretical stellar models with variable G /Brans-Dicke cosmological theory/ in isochrones of one, three and five billion years

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baicz..33..180p&link_type=gif

Astronomical Institutes of Czechoslovakia, Bulletin, vol. 33, no. 3, 1982, p. 180-187.

Astronomy and Astrophysics

Astronomy

1

Cosmology, Stellar Evolution, Stellar Gravitation, Stellar Models, Gravitational Constant, Hertzsprung-Russell Diagram, Nuclear Reactions, Stellar Luminosity, Stellar Mass

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