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Symposium - International Astronomical Union, Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies

Volume 143 - 1991
Contents

Page 8 of 8

Session VIII. Inventory and Distribution

  • Wolf-Rayet Galaxies

  • William D. Vacca, Peter S. Conti
  • Published online by Cambridge University Press:
    03 August 2017, p. 656
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    • NASA ADS Abstract Service

  • Computer Simulation of the Evolution of Active AGN: Single Supermassive Star Versus a Cluster of Massive WR Stars

  • R. Spurzem, K. Herzig
  • Published online by Cambridge University Press:
    03 August 2017, pp. 657-658
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  • The evolution of gas and stars in galactic nuclei is reconsidered and numerical models of early evolutionary phases of galactic nuclei are discussed, in particular the evolution of a supermassive gaseous object as a hypothetical precursor of a supermassive black hole.

Session IX. Summary

  • Summary of Symposium

  • Peter S. Conti
  • Published online by Cambridge University Press:
    03 August 2017, pp. 661-668
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  • “It is a significant fact that the emission and absorption lines of Wolf-Rayet spectra cannot be regarded as being formed in one body of gas at one representative temperature and pressure” (Underhill 1968)

    “I think it fair to say that the demonstration of… diversity has brought the Wolf-Rayet stars from being a curiosity to being an important part of the ‘main stream’ evolution of all massive stars” (Smith 1982)

Other

  • Closing Remarks by the Rector of Universitas Udayana, Denpasar

  • I.G.N.P. Adnyana
  • Published online by Cambridge University Press:
    03 August 2017, p. 669
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  • Object Index

  • Published online by Cambridge University Press:
    03 August 2017, pp. 671-680
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Front Matter

  • IAS volume 143 Cover and Front matter

  • Published online by Cambridge University Press:
    03 August 2017, pp. f1-f14
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Back Matter

  • IAS volume 143 Cover and Back matter

  • Published online by Cambridge University Press:
    03 August 2017, p. b1
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Page 8 of 8