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Late Stages of Stellar Evolution

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ISO Science Legacy

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Abstract

A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH+.

Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.

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Authors and Affiliations

  1. Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200B, B-3001, Leuven, Belgium

    Joris A. D. L. Blommaert

  2. NASA Ames Research Center, MS 245-6, Moffett Field, CA, 94035, USA

    Jan Cami

  3. N. Copernicus Astronomical Center, Rabiánska 8, 87-100, Toruńn, Poland

    Ryszard Szczerba

  4. Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK

    Michael J. Barlow

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  1. Joris A. D. L. Blommaert
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  2. Jan Cami
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  3. Ryszard Szczerba
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  4. Michael J. Barlow
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Editors and Affiliations

  1. European Southern Observatory, Garching, Munich, Germany

    Catherine Cesarsky

  2. European Space Agency, Madrid, Spain

    Alberto Salama

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Blommaert, J.A.D.L., Cami, J., Szczerba, R., Barlow, M.J. (2005). Late Stages of Stellar Evolution. In: Cesarsky, C., Salama, A. (eds) ISO Science Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3844-5_10

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