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Sur la Validité de la Relation Masse-Luminosité dans Le Calcul Des Masses des Étoiles

  • Paul Couteau (a1)

Extract

Les travaux sur les parallaxes dynamiques sont peu nombreux; les plus rÉcents remontent dÉjá loin dans le passÉ (Russell et Moore, 1940; Barbier, 1936; Baize et Romani, 1946; et Strand, 1953). L'idÉe directrice est toujours la même: associer la troisieme loi de Kepler et une relation masse-luminosité.

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References

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Baize, P.: 1947, ‘Les masses des etoiles doubles visuelles et la relation empiriquemasse-luminosite', Bull. Astron. 13, 123.
Baize, P. et Romani, L.: 1946, ‘Formules nouvelles pour le calcul des parallaxes dynamiques des couplex orbitaux', Ann. Astrophys. 9, 13.
Barbier, D.: 1936, ‘Les parallaxes dynamiques des etoiles doubles', Act. Sci. Indust. No. 348.
Russell, H. N. and Moore, Ch. E.: 1940, The Masses of the Stars, University of Chicago Press.
Strand, K. Aa.: 1953, ‘Dynamical Parallaxes from Photographic Observations', Astron. J. 58, 229.

Sur la Validité de la Relation Masse-Luminosité dans Le Calcul Des Masses des Étoiles

  • Paul Couteau (a1)

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