Titlebook: Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems; A. H. Batten Book 1973 International Astronomical Union 197

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https://doi.org/10.1007/978-4-431-55726-5ss loss in the past: Algol-like semidetached binaries, some shell stars (AX Mon), some binary X-ray sources (Cen X-3, Her X-l), the recurrent nova T CrB, helium-rich binaries . Sgr and KS Per, and the symbiotic variables..Algol-like binaries like U Sge cannot be products of a conservative case A of

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John W. Hadden,Ronald G. Coffeyouched upon many items, some of them apparently not strictly connected with the subject of the meeting but helpful to clarify the picture related to close binaries and aimed at establishing differences with single stars, whenever possible. Therefore, my task would be somewhat difficult it if were no

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Expanding Envelopes of Stars,se is complicated by the known binary nature of many Wolf-Rayet stars. Other groups of stars possessing envelope-like structures — U Gem stars and old novae, symbiotic stars, and T Tauri stars — are briefly mentioned. The problems of stellar envelopes, first listed by Struve thirty years ago, are still unsolved.

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Book 1973 Observatory to the Executive Committee of the International Astronomical Union in the summer of 1969. It received the support of the presidents of Commissions 29 (Stellar Spectra), 30 (Radial Velocities), 36 (Stellar Atmospheres), and 42 (Photometric Double Stars). Approval in principle was given b

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Immunopathology of Immune Complex Disease,es by the action of the radiation force..In (3) the large differences in the coronal properties of stars of different chemical composition are emphasized. We draw attention to the partially unexplored but probably very interesting properties of coronae of helium-rich stars.

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Problems of Gaseous Motion Around Stars,ng and the orbital period is discussed. The relation of circumstellar streams to period changes is mentioned. Finally, the influence of magnetic fields on the circumstellar material and the system is discussed.

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