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Symposium - International Astronomical Union, Asymptotic Giant Branch Stars

Volume 191 - 1999
Contents

Page 5 of 5

Part 7. Summary

  • Recent and Future Studies of Circumstellar Matter – A Snapshot

  • M. Jura
  • Published online by Cambridge University Press:
    25 May 2016, pp. 603-610
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    • NASA ADS Abstract Service

  • At this meeting, powerful new images and spectroscopy of AGB stars were presented. Theoretical models have advanced, and we are learning more from studies of the pre-solar grains isolated from meteorites.

    We suggest that several mass loss mechanisms may be operating in AGB stars: current images imply both spherical winds and highly flattened outflows. There are good arguments that in some cases, a companion may be critical in driving the final outflow. In the near future, a number of extremely powerful new instruments and techniques will be available that will lead to a much deeper understanding of these systems.

Other

  • Poster Contributions

  • Published online by Cambridge University Press:
    25 May 2016, pp. 611-620
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  • Quotations from AGB98

  • Published online by Cambridge University Press:
    25 May 2016, pp. 621-624
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  • Author index

  • Published online by Cambridge University Press:
    25 May 2016, pp. 625-627
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  • Object index

  • Published online by Cambridge University Press:
    25 May 2016, pp. 628-630
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  • Subject index

  • Published online by Cambridge University Press:
    25 May 2016, pp. 631-632
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Front matter

  • IAS volume 191 Cover and Front matter

  • Published online by Cambridge University Press:
    25 May 2016, pp. f1-f12
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Back matter

  • IAS volume 191 Cover and Back matter

  • Published online by Cambridge University Press:
    25 May 2016, p. b1
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Page 5 of 5