Algols; Proceedings of the 107th IAU Colloquium, Sidney, Canada, Aug. 15-19, 1988

Astronomy and Astrophysics – Astronomy

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Aerospace Sciences, Conferences, Accretion Disks, Eclipsing Binary Stars, H Alpha Line, Light Curve, Mass Flow, Mass Transfer, Radio Emission, Signal To Noise Ratios, Star Formation, Stellar Envelopes, Stellar Evolution, Stellar Mass, Stellar Spectrophotometry, Supergiant Stars, Ultraviolet Astronomy

Scientific paper

Papers concerning Algols, or semidetached binaries with nondegenerate components, are presented, covering topics such as H-alpha emitting regions and photometric effects of Algol accretion disks, time-resolved spectroscopy of Algol accretion disks, polarizing gas at small optical depths around Algols, mass flow in interacting binaries, interactions between V356 Sagitarii and Beta Lyrae, and theoretical models of Algol disks. Other topics include the formation and evolution of Algols, the fundamental parameters of W Serpentis stars, the relation between RS Canum Venaticorum and Algol, simulated Algol data, the effects of magnetic fields on Algols, ST Carinae, QS Aquilae, BF Centauri in NGC 3766, RS Vulpeculae, RY Scuti, RZ Eridani, and oscillations of CI Aurigae and AQ Tauri. In addition, papers are given concerning the dust shell around V718 Scorpii, synthetic light curve analysis of BX Andromedae and RR Leporis, spectroscopy of KX Andromedae and RX Cassiopeiae, modifications of the Wilson-Devinney Program, transient color changes of Algols, and rotation rates for RW Monocerotis and RW Tauri.

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