Skip to main content

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 223))

Abstract

The Hipparcos space mission is one of the most fascinating experiment in astrometry never realised. Its importance from a general point of view has not to be recalled but it may be interesting to here examine the part it might have for double star astronomy and more precisely for our research on the evolution of the binaries.

In this introductory lecture, we first recall the theories that have been proposed in the past and how we to-day may consider the problem on the basis of our present knowl- edge from a somewhat personal point of view. In that respect we shall here consider the histogram of the real separations of the components, the period-eccentricity relation, the mass-ratio distribution and the HR diagram for binaries. The evolution by secular mass- loss is finally considered with its different possible consequences.

Finally the Hipparcos contribution to binary star evolution is discussed on the basis of the different output of the satellite, as the positions (absolute and relative), the parallaxes, the proper motions, the photometric data and the discovery of new systems.

From a personal point of view, it appears that beside the parallaxes (the original duty of the mission), the most important result of the satellite is the discovery of new systems due to the general survey of the sky by the mission as well as the photometric data that will be provided for the individual components of the close pairs.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 169.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 219.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 219.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Similar content being viewed by others

References

  • ABT, H.A. & Levy, S.G.: 1976, Multiplicity among solar-type stars; Ap.Journal. S.S., 30, pp.273–306.

    Article  ADS  Google Scholar 

  • ABT, H.A. & Levy, S.G.: 1978, Binaries among B2-B5 IV,V absorption and emission stars, Ap.Journal. S.S., 36, pp.241–258.

    Article  ADS  Google Scholar 

  • ABT, H.A.: 1988, Visual binary separations as functions of primary types, ages and locations, Astrophysics and Space Science, 142, pp. 111–121.

    Article  ADS  Google Scholar 

  • ARCORAGI, J.P., Bonnell, I., Martel, H., Bastien, P. & Benz, W.: 1991, Formation of binary and multiple star systems, Bulletin of the American Astronomical Society, 23, p. 1266.

    ADS  Google Scholar 

  • BAIZE, P.: 1932, L’origine et l’évolution des étoiles doubles,. Revue Scientifique, 70, n°14, 23 juillet, pp.418–426.

    Google Scholar 

  • BATTEN, A.H.: 1992, Towards a comprehensive view of binary and multiple systems, IAU Colloquium 135, Complementary approaches to double and multiple star research, Astronomical Soc. of the Pacific, Conference Series, 32, pp.586–592.

    ADS  Google Scholar 

  • BLEKSLEY, A.E.H.: 1934, Loss of mass in binary systems, Nature, 133, 613.

    Article  ADS  Google Scholar 

  • BONEFF, N.: 1951, Sur l’origine des étoiles doubles, Annuaire de la Faculté des Sciences, Physique et Mathématiques, 47, 191–199.

    Google Scholar 

  • BOSLER, J.: 1928, Cours d’Astronomie, III Astrophysique, Librairie Scientifique Hermann & Cie, pp. 580–586.

    MATH  Google Scholar 

  • BOSS, A.P.: 1992, The fragmentation mechanism, Astronomical Society of the Pacifíc, Conference series, 32, pp.195–205.

    ADS  Google Scholar 

  • CAMPBELL, W.W.: 1910, Second catalogue of spectroscopic binary stars, Lick Observatory Bulletin, 6, pp.17–54.

    ADS  Google Scholar 

  • CHIARA, L.: 1955–56, Casi in cui nel problema dei due corpi di massa decrescente l’eccentricita varia in raggione inversa delia massa, Atti dell’accademia di Scienze, Lettere e Arti di Palermo, série 4, 16, Pubbl. Dell’osservatorio astron. di Palermo, N.S. 10, n°8.

    Google Scholar 

  • CLARKE, C.J.: 1992, The formation of binary stars, Proceedings of the workshop.: Binaries as traces of Stellar Formation, Ed. Duquennoy, A. & Mayor, M., Cambridge University Press, Cambridge.

    Google Scholar 

  • COUTEAU, P.: 1967, Relation masse-luminosité et diagram H-R dans le cas des binaires, Comptes Rendus du Colloque UAI On the Evolution of Double Stars Comm. de l’Obs. Royal, de Belg., Série B, n°17, pp.181–188.

    Google Scholar 

  • DARWIN, G.H.: 1886, On Jacobi’s figure of equilibrium for a rotating mass of fluid, Proceedings of the Royal Society 41, pp.319–336.

    Google Scholar 

  • Also in.: Scientifíc Papers, 1910, 3, pp. 119–134, Cambridge University Press.

    Google Scholar 

  • DARWIN, G.H.: 1887, On figures of equilibrium of rotating mass of fluid, Proceedings of the Royal Society, 42, pp.359–362.

    Google Scholar 

  • Also in.: Scientifíc Papers, 1910, 3, pp. 135–185, Cambridge University Press.

    Google Scholar 

  • DARWIN, G.H.: 1900, Address delivered by the President, Monthly Notices of the R. Astron. Soc, 60, pp.406–415.

    ADS  Google Scholar 

  • DARWIN, G.H.: 1910, Scientific papers, Vol. III, Figures of equilibrium of rotating liquid and geophysical investigations, Cambridge University Press, Cambridge, 527 pp.

    Google Scholar 

  • DARWIN, G.H.: 1911, The Tides and kindred phenomena in the solar system, Third edition, Chapter XIX, pp. 353–402, Ed. John Murray, London.

    Google Scholar 

  • De GREVE, J.P. & De Loore C: 1972, Stellar winds and mass-loss of a rotating star, Astrophysics and Space Science, 18, pp. 128–134.

    Article  ADS  Google Scholar 

  • DOBERCK, W.: 1878, On double star orbits, Astronomische Nachrichten, 91, pp.317–318.

    Article  ADS  Google Scholar 

  • DOBERCK, W.: 1898, On double star orbits.: their periods and eccentricities, Astronomische Nachrichten, 147, pp.251–252.

    Article  ADS  Google Scholar 

  • DOMMANGET, J.: 1963, Recherches sur l’évolution des étoiles doubles par voie statistique et par application de la mécanique des masses variables, Annales de l’Obs. R. de Belg. 3éme série, 9, 5, pp.213–304.

    Google Scholar 

  • DOMMANGET, J.: 1964, Les étoiles doubles et l’évolution stellaire, Ciel et Terre, 80, pp.315–338, Communication de l’Obs. R. de Belg. n°232.

    ADS  Google Scholar 

  • DOMMANGET, J.: 1968, La cinématique des couples stellaires visuels dans le voisinage du Soleil, Bulletin de l’Obs. Royal de Belg., 6, pp.246–249.

    ADS  Google Scholar 

  • DOMMANGET, J.: 1970, La fréquence des étoiles doubles dans l’univers sidéral, Ciel et Terre, 86, pp.463–485

    ADS  Google Scholar 

  • COMM. de L’OBS. Royal de Belg. série B, n°56, pp. 463–485.

    Google Scholar 

  • Dommanget, J.: 1971, La distribution des distances de séparation des étoiles doubles et ses enseignements, Sciences, tome II, n°3, pp.151–160

    Google Scholar 

  • COMM. de L’OBS. Royal de Belg., série B, n°70.

    Google Scholar 

  • DOMMANGET, J.: 1981, Is this diagram an argument for binary orbital evolution due to mass-loss? Astrophysics and Space Science Library, 89, pp.507–513

    ADS  Google Scholar 

  • Comm. de l’Obs. Royal de Belg., série B, n°119.

    Google Scholar 

  • DOMMANGET, J.: 1982a, A mass-eccentricity correlation in spectroscopic and visual binary orbits, Astrophysics and Space Science Library, 98, pp. 119–122.

    ADS  Google Scholar 

  • DOMMANGET, J.: 1982b, L’astronomie des étoiles doubles á l’heure de l’astrométrie spatiale, L’Astronomie, 96, pp.15–27

    ADS  Google Scholar 

  • Comm. de l’Obs. Royal de Belg., série B, n°125.

    Google Scholar 

  • DOMMANGET, J.: 1983a, La constante des aires des binaires visuelles orbitales dans le diagram HR, Comptes Rendus sur les Journées de Strasbourg, Les étoiles binaires dans le diagram H.R., 5éme réunion, pp. 39–43.

    Google Scholar 

  • DOMMANGET, J.: 1983b, L’astronomie des étoiles doubles face á la mission du satellite astrométrique Hipparcos, Comm. de l’Obs. Royal de Belg., série B, n°127.

    Google Scholar 

  • DOMMANGET, J.: 1988, The space arrangement of the orbital planes of the visual double stars, Astrophysics and Space Science, 142, pp.171–176.

    Article  ADS  Google Scholar 

  • DOMMANGET, J. & LAMPENS, P.: 1993, How double star astronomy may develop after Hipparcos, Astrophysics and Space Science, 200, pp.221–238

    Article  ADS  Google Scholar 

  • Comm. de l’Obs. R. de Belg. Série B, n°161.

    Google Scholar 

  • DOMMANGET, J. & NYS, O.: 1994, Catalogue of the Components of Double and Multiple stars (CCDM), Communication de l’Observatoire R. de Belg. Série A, n°115, pp.26.

    Google Scholar 

  • DOMMANGET, J.: 1995, Is this orbit really necessary ? (III) Astronomy & Astrophysics, (Research Note) 301, pp. 919–921.

    ADS  Google Scholar 

  • DUFOUR, Ch.: 1930, Sur l’accélération séculaire du mouvement de la Lune, Comptes Rendus, Académie des Sciences de Paris, 62, pp. 840–842.

    Google Scholar 

  • DUQUENNOY, A. & Mayor, M.: 1991a, Multiplicity among solar-type stars in the solar neighbourhood I.: Coravel radial velocity observations of 291 stars, Astronomy & Astrophysics, S.S., 88, pp. 281–324.

    ADS  Google Scholar 

  • DUQUENNOY, A. & Mayor, M.: 1991b, Multiplicity among solar-type stars in the solar neighbourhood II.: Distribution of the orbital elements in an unbiased sample, Astronomy & Astrophysics, 248, pp. 485–524.

    ADS  Google Scholar 

  • DUQUENNOY, A. & Mayor, M.: 1992, Binaries as traces of Stellar Formation, Proceedings of a workshop in Switzerland, Cambridge University Press, Cambridge.

    Google Scholar 

  • EDDINGTON, A.S.: 1923, On the relation between the masses and luminosities of the stars, Monthly Notices of the R. Astron. Soc, 84, pp. 308–332.

    ADS  Google Scholar 

  • FESENKOV, V.G.: 1952, Le rayonnement corpusculaire, comme facteur d’évolution du Soleil et des étoiles, Transactions of the International Astronomical Union, 8, p. 702–714.

    Google Scholar 

  • FINSEN, W.S.: 1936, The apparent statistical relation between period and eccentricity in visual binary orbits, Monthly Notices of the R. Astron. Soc, 96, pp. 862–866.

    ADS  Google Scholar 

  • FROESCHLE, M.: 1995, La mission Hipparcos, Une belle moisson de résultats, Bulletin de l’Association pour le Développement International de l’Observatoire de Nice, 29, pp.15–19.

    Google Scholar 

  • GIANNUZZI, M.A.: 1989 -Visual binary systems in the solar neighbourhood.: a question of their separations, Astrophysics and Space Science, 161, pp. 241–246.

    Article  ADS  Google Scholar 

  • GLIESE, W. & Jahreiss, H.: 1988, The third catalogue of nearby stars with special emphasis on wide binaries, Astrophysics and Space Science, 142, pp.49–56.

    Article  ADS  Google Scholar 

  • HALB WACHS, J.L.: 1983, Binaries among the bright stars.: estimation of the bias and study of the main-sequence stars, Astronomy & Astrophysics, 128, pp. 399–404.

    ADS  Google Scholar 

  • HALBWACHS, J.L.: 1986, Binaries among bright stars.: systems with evolved primary components and their relation to the properties of main-sequence binaries, Astronomy & Astrophysics, 168, pp. 161–158.

    ADS  Google Scholar 

  • HEINTZ, W.: 1967, Some results of binary statistics, in.: “On the evolution of double stars” Comm. de VObs. Royal de Belg. Série B, 17, pp. 49–52.

    Google Scholar 

  • HEINTZ, W.: 1969, A statistical study of binary stars, Journal of the Royal Astronomical Society of Canada, 63, pp.275–298.

    ADS  Google Scholar 

  • HICKS, W.M.: 1882, Reports on the state of science, Fluid ellipsoid and sphere under their own attractions, Report of the fifty-second meeting of the British Association for the Advancement of Science, Ed. John Murray, London, pp.57–62.

    Google Scholar 

  • HOGEVEEN, S.J.: 1990, The mass-ratio distribution of visual binary stars, Astrophysics and Space Science, 173, pp.315–342.

    Article  ADS  Google Scholar 

  • HOYLE, F.: 1953, On the fragmentation of gas clouds into galaxies and stars, Astroph. Journal, 118, pp.513–528.

    Article  ADS  Google Scholar 

  • JEANS, J.H.: 1919, Problems of cosmogony, Stellar dynamics,

    Google Scholar 

  • JEANS, J.H.: 1924, Cosmogonie problems associated with a secular decrease of mass, Monthly Notices of the R. Astron. Soc. 85, pp.2–11.

    ADS  Google Scholar 

  • JEANS, J.H.: 1925, The effect of varying Mass on a binary system, Monthly Notices of the R. Astron. Soc. 85, pp.912–914.

    ADS  Google Scholar 

  • JEANS, J.H.: 1928, Astronomy and Cosmogony, Cambridge University Press, Cambridge, 420 pp.

    MATH  Google Scholar 

  • JORISSEN, A.: 1984, Tendance évolutive du rapport des masses dans les binaires visuelles, Bulletin de l’Obs. Royal de Belg. 9, fasc.6, pp.325–329.

    ADS  Google Scholar 

  • KELVIN (Lord) (= Sir William Thomson), 1891, On the Sun’s heat, Popular lectures and Addresses, vol I, pp.413–417.

    Google Scholar 

  • KUIPER, G.P.: 1935, Problems of double star astronomy II, Publ. of the Astronomical Soc. of the Pacific, 47, pp.121–150.

    Article  ADS  Google Scholar 

  • KUIPER, G.P.: 1955, On the origin of binary stars, Publ. of the Astronomical Soc. of the Pacific, 67, pp.387–396.

    Article  ADS  Google Scholar 

  • LIOUVILLE, J.: 1834 -Sur la figure d’une masse fluide homog00E9ne, en équilibre, et douée d’un mouvement de rotation, Journal de l’Ecole Royale Polytechnique, 23éme cahier, 14, pp.289–296.

    Google Scholar 

  • LOSS EVA, V.M.: 1938, Le décroissement de la masse et le changement de la somme et du rapport des masses des composantes des systèmes binaires, Russian astronomical Journal, 15, pp.232–247.

    Google Scholar 

  • LYTTLETON, R.A.: 1954, The theoretical basis of the fission theory of binary stars, Transactions of the International Astronomical Union, 8, pp.717–721.

    Google Scholar 

  • LUDENDORFF, H.: 1910, Zur Statistik des spektroskopischen Doppelsterne, Astronomische Nachrichten, 184, pp.373–390.

    Article  ADS  Google Scholar 

  • MAC-LAURIN, C: 1741, De causa physica fluxus et refíuxus maris, Piéces qui ont remporté le prix de l’Académie Royal des Sciences en 1740 sur le flux et reflux de la mer, Paris 1741, pp. 195–233.

    Google Scholar 

  • MARTIN, E.L.: 1934, Sulle variazioni secolari del periastro e dlla eccentricitá secondo una nuova legge di irragiamento della massa per i sistemi binari, Reale statione astronomica e geofísica di Carloforte (Cagliari), No. 30, 16 pp.

    Google Scholar 

  • MAZEH, T. & Goldberg, D.: 1962, The mass-ratio distribution of short-period binaries, Astronomical Society of the Pacifíc, Conference Series, 32, pp.119–126.

    ADS  Google Scholar 

  • MOULTON, F.R.: 1906, An introduction to Astronomy, pp.524–526. The Macmillan Company, London.

    MATH  Google Scholar 

  • MOULTON, F.R.: 1909, Notes on the possibility of fission of a contracting rotating fluid of mass, (in.: Contributions to cosmogony and the fundamental problems of Geology, The tidal and other problems, Ed. The Carnegie Institution of Washington), pp.135–160.

    Google Scholar 

  • Moulton, F.R.: 1931, Astronomy, The Macmillan Company, New York, pp.400–403 and 440–443.

    Google Scholar 

  • MULLER, P.: 1952, Colorimétrie de cinquante et une étoiles doubles, Annales de l’Observatoire de Strasbourg, 5, fasc. 4, pp. 2–31.

    Google Scholar 

  • MULLER, P.: 1967, Comptes Rendus du Colloque UAI On the evolution of double stars; Comm. de l’Obs. Royal de Belg. Série B, n°17, pp.189–190.

    Google Scholar 

  • ÖPIK, E.: 1923, On the luminosity-curve of components of double stars, Publications de l’Observatoire Astronomique de l’Université de Tartu, 25, 5, 28 pp.

    Google Scholar 

  • ÖPIK, E.: 1924, Statistical studies of double stars, Publications de l’Observatoire Astronomique de l’Université de Tartu, 25, 6, 167 pp.

    Google Scholar 

  • PLATEAU, J.: 1843, Mémoire sur les phénoménes que présente une masse liquide libre et soustraite á l’action de la pesanteur, premi00E9re partie, Nouveaux mémoires de l’Académie Royale des Sciences et Belles-Lettres de Bruxelles, 16, 34 pp. + 1 planche.

    Google Scholar 

  • PLAVEC, M.J.: 1982, Evolution of close binary stars.: observational aspects, Astrophysics and Space Science Library, 98, pp. 159–181.

    ADS  Google Scholar 

  • POINCARE, H.: 1911, Leçons sur les hypoth00E9ses cosmogoniques. Librairie Scientifique Hermann et Fils, Paris, 1911, pp. 184–189.

    Google Scholar 

  • RUSSELL, H.N.: 1910, On the origin of binary stars, Astrophysical Journal, 31, 3, pp.185–207.

    Article  ADS  Google Scholar 

  • SCHLESINGER, Fr. & BAKER, R.H.: 1910, A comparative study of spectroscopic binaries, Publications of the Allegheny Observatory, 1, pp.135–161.

    ADS  Google Scholar 

  • SCHMIDT, O.J.: 1945, On the inclination of the planes of double star orbits to the plane of the Galaxy, Comptes Rendus de l’Académie des Sciences de l’U.R.S.S.(NS), 49, pp.16–19.

    Google Scholar 

  • SEE, T.J.J.: 1893, Die Entwickelung der Doppelstern-Systeme, Inaugural-Dissertation zur Erlangung der Doctorwürde von der Philosophischen Facultät der Königlichen Friedrich-Wilhelms-Universität zu Berlin, R.Friedländer & Sohn, Berlin.

    Google Scholar 

  • SEE, T.J.J.: 1896, Researches on the evolution of the stellar systems, tome I, Thos. P. Nichols & Sons, Lynn, Mass. USA.

    Google Scholar 

  • SEE, T.J.J.: 1910, Researches on the evolution of the stellar systems, tome II, Thos. P. Nichols & Sons, Lynn, Mass. USA.

    Google Scholar 

  • SMART, W.M.: 1925, The cosmogonie time-scale and binary stars, Monthly Notices of the R. Astron. Soc, 85, pp.423–433.

    ADS  Google Scholar 

  • STONEY, J.: 1867, On the physical constitution of the sun and stars, Proc. R. Sc. London, 16, pp.25–34.

    Article  Google Scholar 

  • Strand, K.Aa.: 1967, General Introductory lecture to the IAU Colloquium On the evolution of double stars; Comm. de l’Obs. R. de Belg., série B, n°17, pp.19–24.

    Google Scholar 

  • STRUVE, O.: 1950, Stellar evolution, Princeton University Press, 266 pp.

    Google Scholar 

  • Trimble, V.: 1974, On the distribution of binary system mass ratio, Astronomical Journal, 79, pp. 967–973.

    Article  ADS  Google Scholar 

  • TRIMBLE, V.: 1978, q (a) reconsidered, The Observatory, 98, pp.163–166.

    Google Scholar 

  • TRIMBLE, V.: 1986, The angular momentum-vs-mass relation and the distribution of mass ratios for visual binary systems, Astrophysics and Space Science, 126, pp.243–253.

    Article  ADS  Google Scholar 

  • Turon, C & alt.: 1992, The Hipparcos Input Catalogue, ESA SP-1136, 6 volumes.

    Google Scholar 

  • VARSAVSKY, C.M.: 1962, An interpretation of the period-eccentricity relation for double stars, Symposium on Stellar Evolution, Astronomical Observatory, Nat. Univ. of La Plata, pp.173–183.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1997 Kluwer Academic Publishers

About this chapter

Cite this chapter

Dommanget, J. (1997). Hipparcos Contribution to Binary Evolution Research. In: Docobo, J.A., Elipe, A., McAlister, H. (eds) Visual Double Stars: Formation, Dynamics and Evolutionary Tracks. Astrophysics and Space Science Library, vol 223. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1477-3_50

Download citation

  • DOI: https://doi.org/10.1007/978-94-009-1477-3_50

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7161-1

  • Online ISBN: 978-94-009-1477-3

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics