Hostname: page-component-745bb68f8f-cphqk Total loading time: 0 Render date: 2025-01-30T23:47:58.665Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

McDonald, and Webber, B. 1959, Phys. Rev. 115, 194.CrossRefGoogle Scholar
Vera, R.A. 1981a, in Proceedings of the Einstein Centennial Simposium on Fundamental Physics, ed. Moore, S.M., Rodriguez-Vargas, A., Rueda, A., Viollini, G. (Universidad de los Andes, Bogota, Universita di Roma), p. 597. Google Scholar
Vera, R.A. 1981b, Int. J. of Th. Phys. 20, 19.CrossRefGoogle Scholar
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