Abstract
IRAS PSC, LRS, and CPC observations of Wolf-Rayet stars are used as diagnostics of hot circumstellar dust shells, cool dust in WR ring nebulae, the Ne/He abundance ratio, and the interstellar extinction. In two cases the IR energy distributions indicate WR planetary nucleus status rather than Population-I WR status.
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van der Hucht, K.A., Jurriens, T.A., Olnon, F.M., Thé, P.S., Wesselius, P.R., Williams, P.M. (1986). IRAS Observations of Wolf-Rayet Stars. In: Israel, F.P. (eds) Light on Dark Matter. Astrophysics and Space Science Library, vol 124. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4672-9_16
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DOI: https://doi.org/10.1007/978-94-009-4672-9_16
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