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Properties of Post-AGB Stars with Iras Colors Typical of Planetary Nebulae

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Post-AGB Objects as a Phase of Stellar Evolution

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 265))

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Abstract

We have investigated the infrared properties of a sample of objects with IRAS colors typical of planetary nebulae. The selected objects have not yet evolved to the planetary nebula stage since they have no detectable radio continuum emission and they are therefore likely post-AGB stars.

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References

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Author information

Authors and Affiliations

  1. Royal Observatory of Belgium, Ringlaan 3, 1180, Brussels, Belgium

    Griet C. Van de Steene

  2. CITA, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada

    Peter A. M. van Hoof

  3. RSAA, Australian National University, Canberra, ACT 0200, Australia

    Peter R. Wood

Authors
  1. Griet C. Van de Steene
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  2. Peter A. M. van Hoof
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  3. Peter R. Wood
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Editor information

Editors and Affiliations

  1. Nicolaus Copernicus Astronomical Center, Toruń, Poland

    Ryszard Szczerba  & Sławomir K. Górny  & 

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© 2001 Springer Science+Business Media Dordrecht

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Van de Steene, G.C., van Hoof, P.A.M., Wood, P.R. (2001). Properties of Post-AGB Stars with Iras Colors Typical of Planetary Nebulae. In: Szczerba, R., Górny, S.K. (eds) Post-AGB Objects as a Phase of Stellar Evolution. Astrophysics and Space Science Library, vol 265. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9688-6_5

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  • DOI: https://doi.org/10.1007/978-94-015-9688-6_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5758-7

  • Online ISBN: 978-94-015-9688-6

  • eBook Packages: Springer Book Archive

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