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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
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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
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