Astrophysics and Space Science

, Volume 170, Issue 1–2, pp 263–265 | Cite as

Galactic structure parameters from radial velocities of young stars

  • F. Comerôn
  • J. Torra
Structure and Evolution of Galaxies


Radial velocities of OB stars are utilised in order to determine the values of some galactic structure parameters in the solar neighbourhood.


Radial Velocity Young Star Solar Neighbourhood Galactic Structure 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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  1. Brosche, P.: 1966,Veröff. des Astronomisches Rechen-Institut, No. 17, Heidelberg.Google Scholar
  2. Elmegreen, D. M.: 1987, in H. Van Wördenet al. (eds.), “The Milky Way’,IAU Symp. 106, 255.Google Scholar
  3. Figueras, F.: 1986, Ph.D. Thesis, University of Barcelona.Google Scholar
  4. Frogel, J. A. and Stothers, R.: 1977,Astron. J. 82, 890.Google Scholar
  5. Kerr, F. J. and Lynden-Bell, D.: 1986,Monthly Notices Roy. Astron. Soc. 221, 1023.Google Scholar
  6. Ochsenbein, F.: 1980,Bull. Inf. CDS 19, 74.Google Scholar
  7. Robin, A. and Crézé, M.: 1986,Astron. Astrophys. 157, 71.Google Scholar
  8. Rohlfs, K.: 1977,Lectures in Density Waves Theory, Springer-Verlag, Berlin.Google Scholar

Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • F. Comerôn
    • 1
  • J. Torra
    • 1
  1. 1.Departament de Física de l'Atmosfera, Astronomia i AstrofisicaUniversitat de BarcelonaSpain

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