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A New Model for the Structure and Evolution of Main Sequence Stars

Published online by Cambridge University Press:  12 April 2016

Rafael A. Vera
Rafael A. Vera*
Affiliation:
Departamento de Fisica, Facultad de Ciencias, Universidad de Concepcion, Casilla 3C, Concepcion, Chile

Abstract

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From both astronomical facts and theory it is inferred that the primary energy of main sequence stars most probably comes from gravitational work around a neutron star. The new mechanisms involved can in principle account for the observed facts, including those unconsistent with conventional models.

Type
XI. Supplement
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 798 - 800
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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Vera, R.A. 1986, in Proceedings of the IV Marcel Grossmann Meeting on General Relativity, ed. Ruffini, R., Elsevier Science Publications B V, p. 1743. Google Scholar