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LSS 4005 and NaSt1, two Galactic Ofpe/WN or B[e] objects*

Published online by Cambridge University Press:  12 April 2016

K.A. van der Hucht ,
P.M. Williams ,
A.M. van Genderen ,
P. Mulder  and
W.J. Zealey
K.A. van der Hucht
Affiliation:
SRON Space Research Utrecht, The Netherlands
P.M. Williams
Affiliation:
Royal Observatory, Edinburgh, Scotland, U.K.
A.M. van Genderen
Affiliation:
Leiden Observatory, The Netherlands
P. Mulder
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
W.J. Zealey
Affiliation:
Department of Physics, University of Wollongong, Australia

Extract

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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.

Type
Section II: Poster Papers, A Brief List of Catalogs, and Index
Information
International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 301 - 302
Copyright
Copyright © Kluwer 1989

Footnotes

*

Based on observations collected at the European Southern Observatory (La Silla, Chile), the United Kingdom Infrared Telescope (Mauna Kea, Hawaii, USA) and the Anglo-Australian Observatory (Epping, NSW, Australia)

References

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