Experientia

, Volume 1, Issue 5, pp 127–136 | Cite as

Le problème des étoiles doubles

  • G. Tiercy
Article

Summary

“A review is given of what we know of binary stars. Leaving out the historical development, the difficulties are shown, which astronomers encountered in their studies of visual as well as spectroscopic or photometric binaries. Thus the reader gets an idea of the methods used both for observing and for explaining the existence of these double stars.

The importance of this problem for modern cosmology and for theoretical physics is pointed out.”

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. 1.
    Handbuch der Astrophysik, Band VI (1928); chap. IV: Double and multiple Stars, byF. C. Henroteau, Ottawa;Ch. André, Traité d'astronomie stellaire, vol. II; Paris (1900);G. Armellini, Astronomia siderale, vol. II; Bologna (1931);T. J. J. See, Researches on the evolution of the stellar systems, Lynn (1896).Google Scholar
  2. 1.
    Connaissance des Temps pour (1830).Google Scholar
  3. 1.
    Kowalsky,Procès-verbaux de l'Université impériale de Kasan (1873).Google Scholar
  4. 2.
    Zwiers,Astronomische Nachrichten, Nr. 3336 (1896).Google Scholar
  5. 3.
    Hellerich,Astronomische Nachrichten, Nr. 5348 (1925).Google Scholar
  6. 4.
    Henroteau-Stewart,Popular Astronomy (1925).Google Scholar
  7. 1.
    S. Glasenapp,Monthly Notices of the R.A.S., vol. 49.Google Scholar
  8. 2.
    T. J. J. See, loc. cit.Google Scholar
  9. 3.
    VoirAitken, The binary Stars, New York (1918).Google Scholar
  10. 1.
    John Herschel, A Catalogue of 10300 multiple and double Stars;Memoirs of the Royal Astronomical Society (1874). —Burnham, A general Catalogue of double Stars, published bythe Carnegie Institution of Washington (1906); etc.Google Scholar
  11. 1.
    C. Niven,Monthly Notices of R.A.S. (1874);C. Pickering,Proceedings of the American Academy of Arts and Science (1880);T. See,Astronomische Nachrichten, Nr. 3314 (1896).Google Scholar
  12. 2.
    Astronomische Nachrichten, Nr. 3510 (1898).Google Scholar
  13. 1.
    Bessel, Über Veränderlichkeit der eigenen Bewegung der Fixsterne,Astronomische Nachrichten (1844).Google Scholar
  14. 1.
    C. Pickering, A new class of binary stars.Monthly Notices of the R.A.S. (1890).Google Scholar
  15. 1.
    Lick Bulletin 6 (1910).Google Scholar
  16. 2.
    Lick Bulletin 11 (1924).Google Scholar
  17. 4.
    Astronomische Nachrichten, Nr. 3242 (1895).Google Scholar
  18. 5.
    Astrophysical Journal (1902 et 1914).Google Scholar
  19. 6.
    Publ. of the Astronomical Society of the Pacific (1917).Google Scholar
  20. 7.
    Publ. of the Allegheny Observatory (1910).Google Scholar
  21. 1.
    Astronomische Nachrichten, Nr. 3051 (1891).Google Scholar
  22. 1.
    Monthly Notices (1906).Google Scholar
  23. 2.
    Astrophysical Journal (1911 et 1912).Google Scholar
  24. 3.
    Astrophysical Journal (1912).Google Scholar
  25. 4.
    Contributions Princeton University Observatory (1930).Google Scholar
  26. 1.
    A. S. Eddington, The internal constitution of the Stars, Cambridge (1926).Google Scholar
  27. 1.
    H. Poincaré, Electricité et optique, Paris (1901).Google Scholar
  28. 2.
    S. Zaremba, La théorie de la relativité et les faits observés,Journal de Mathématiques (1922).Google Scholar
  29. 3.
    H. Varcollier, Propagation ellipsoïdale, relativité, quanta, Alger (1942.)Google Scholar
  30. 4.
    P. Dive, L'électro-optique dans le temps universel, Paris (1941).Google Scholar
  31. 5.
    G. Tiercy, Les binaires à éclipses, la vitesse de la lumière et les théories relativistes;Publ. de l'Observ. de Genève, fasc. 36, (1941). — A propos de la conclusion qu'on peut tirer du problème des étoiles doubles.Archives des sc. phys. et nat., Genève (1942).Google Scholar
  32. 1.
    Cette théorie de la division a été soutenue notamment par:H. Poincaré, Leçons sur les hypothèses cosmogoniques, Paris (1913);H. N. Russell, The Origin of Binary Stars.Astrophysical Journal (1910);F. H. Jeans, Astronomy and Cosmogony, Cambridge (1929).Google Scholar
  33. 2.
    Cette hypothèse, combinée avec la théorie des marées, a été défendue parMoulton etChamberlin et appliquée au système solaire (1914 et 1916).Google Scholar
  34. 3.
    Cette hypothèse de la capture a été défendue notamment parT.J.J. See, Researches on the Evolution of stellar Systems; Lynn (U.S.A.) (1910).Google Scholar

Copyright information

© Birkhäuser Verlag 1945

Authors and Affiliations

  • G. Tiercy
    • 1
  1. 1.Genève

Personalised recommendations