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LSS4005 and NaSt1, Two Galactic Ofpe/WN or B[e] Objects

  • K. A. van der Hucht
  • P. M. Williams
  • A. M. van Genderen
  • P. Mulder
  • W. J. Zealey
Part of the Astrophysics and Space Science Library book series (ASSL, volume 157)

Abstract

Optical and IR spectroscopy of two galactic objects previously considered to be extreme late WN stars (van der Hucht et al., 1984), LSS4005 (formerly tentatively listed as WR85a) and NaStl (WR122), show both objects not to be WR stars, but Ofpe/WN- or B[e]-like objects.

Keywords

Emission Line European Southern Observatory Dust Envelope Circumstellar Dust Hell Emission 
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.

References

  1. van der Hucht, K.A., Williams, P.M., Thé, P.S.: 1984, in: A. Maeder & A. Renzini (eds.), Observational Tests of the Stellar Evolution Theory, Proc. IAU Symp. 105 (Dordrecht: Reidel), p. 273Google Scholar
  2. Williams, P.M., van der Hucht, K.A., Thé, P.S.: 1987, Astron. Astrophys. 182, 91ADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • K. A. van der Hucht
    • 1
  • P. M. Williams
    • 2
  • A. M. van Genderen
    • 3
  • P. Mulder
    • 4
  • W. J. Zealey
    • 5
  1. 1.SRON Space Research UtrechtThe Netherlands
  2. 2.Royal ObservatoryEdinburghScotland, UK
  3. 3.Leiden ObservatoryThe Netherlands
  4. 4.Kapteyn Astronomical InstituteGroningenThe Netherlands
  5. 5.Department of PhysicsUniversity of WollongongAustralia

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