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Observational Contrains on Collimation Mechanisms in RU Lupi

  • S. Lamzin
  • F. Giovannelli
  • C. Rossi
  • L. Errico
  • A. A. Vittone
  • G. S. Bisnovatyi-Kogan
  • V. G. Kurt
  • E. K. Sheffer
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 186)

Abstract

A large campaign of multifrequency observations of extreme T Tauri star RU Lupi was performed from 1983 to 1988. We present here main observational results of the campaign and their preliminary interpretation in terms of disk accretion onto an young star with moderately strong global magnetic field.

Keywords

Disk Accretion Young Star Balmer Line Bolometric Luminosity Accretion Column 
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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Copyright information

© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  • S. Lamzin
    • 1
  • F. Giovannelli
    • 2
  • C. Rossi
    • 3
  • L. Errico
    • 4
  • A. A. Vittone
    • 4
  • G. S. Bisnovatyi-Kogan
    • 5
  • V. G. Kurt
    • 5
  • E. K. Sheffer
    • 1
  1. 1.Sternberg Astronomical InstituteMoscowRussia
  2. 2.Space Astrophysical Institute CNRFrascatiItaly
  3. 3.Istituto AstronomicoUniversità di RomaRomaItaly
  4. 4.Osservatorio Astronomico di CapodimonteNapoliItaly
  5. 5.Space Research InstituteMoscowRussia

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