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- catalog abstract "There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures.".
- catalog contributor b11259905.
- catalog contributor b11259906.
- catalog contributor b11259907.
- catalog contributor b11259908.
- catalog created "c1999.".
- catalog date "1999".
- catalog date "c1999.".
- catalog dateCopyrighted "c1999.".
- catalog description "I Observation of Non-spherical Winds: Rotationally Modulated Winds of O-Stars -- Rotationally Modulated Winds of BA-Type Supergiants -- Using Spectropolarimetry to Determine Envelope Geometry and Test Variability Models for Hot Star Circumstellar Envelopes -- Disks of Classical Be Stars -- II Theory of Non-spherical Winds: Wind-Compressed Disks -- Non-spherical Radiation-Driven Wind Models -- Radiation-Driven Disk Winds -- III Variable Winds: O-Star Wind Variability in the Ultraviolet and Optical Range -- X-Ray Evidence for Wind Instabilities -- IV Theories of Wind Variations: The Line-Driven Instability -- Co-Rotating Interaction Regions -in 2DHot-Star Wind Models with Line-Driven Instability -- V Pulsation: Pulsations in O-Stars -- Nonradial Pulsations of BA Supergiants and Be Stars -- Theory of Pulsational Instabilities of Hot Stars -- VI Evolutionary Aspects: The Evolution of Non-spherical and Non-stationary Winds of Massive Stars -- Rotation and Anisotropic Losses of Mass and Angular Momentum. lfvjbö v övj bafökvj bafövk jbafvö kajfv övkjb övkj bfövk jbfvkö jbvök jbfvlö advsdvl jbsdv ölsjbvd ksvbjd kdvjb kjb.".
- catalog description "Includes bibliographical references and index.".
- catalog description "There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures.".
- catalog extent "xx, 424 p. :".
- catalog hasFormat "Variable and non-spherical stellar winds in luminous hot stars.".
- catalog identifier "3540657029 (acid-free paper)".
- catalog isFormatOf "Variable and non-spherical stellar winds in luminous hot stars.".
- catalog isPartOf "Lecture notes in physics, 0075-8450 ; 523".
- catalog issued "1999".
- catalog issued "c1999.".
- catalog language "eng".
- catalog publisher "Berlin ; New York : Springer,".
- catalog relation "Variable and non-spherical stellar winds in luminous hot stars.".
- catalog subject "523.8/8 21".
- catalog subject "Astronomy.".
- catalog subject "Astrophysics.".
- catalog subject "Early stars Congresses.".
- catalog subject "Physics.".
- catalog subject "QB843.E2 I28 1998".
- catalog subject "Stellar winds Congresses.".
- catalog tableOfContents "I Observation of Non-spherical Winds: Rotationally Modulated Winds of O-Stars -- Rotationally Modulated Winds of BA-Type Supergiants -- Using Spectropolarimetry to Determine Envelope Geometry and Test Variability Models for Hot Star Circumstellar Envelopes -- Disks of Classical Be Stars -- II Theory of Non-spherical Winds: Wind-Compressed Disks -- Non-spherical Radiation-Driven Wind Models -- Radiation-Driven Disk Winds -- III Variable Winds: O-Star Wind Variability in the Ultraviolet and Optical Range -- X-Ray Evidence for Wind Instabilities -- IV Theories of Wind Variations: The Line-Driven Instability -- Co-Rotating Interaction Regions -in 2DHot-Star Wind Models with Line-Driven Instability -- V Pulsation: Pulsations in O-Stars -- Nonradial Pulsations of BA Supergiants and Be Stars -- Theory of Pulsational Instabilities of Hot Stars -- VI Evolutionary Aspects: The Evolution of Non-spherical and Non-stationary Winds of Massive Stars -- Rotation and Anisotropic Losses of Mass and Angular Momentum. lfvjbö v övj bafökvj bafövk jbafvö kajfv övkjb övkj bfövk jbfvkö jbvök jbfvlö advsdvl jbsdv ölsjbvd ksvbjd kdvjb kjb.".
- catalog title "Variable and non-spherical stellar winds in luminous hot stars : proceedings of the IAU Colloquium no. 169, held in Heidelberg, Germany, 15-19 June 1998 / B. Wolf, O. Stahl, A.W. Fullerton (eds.).".
- catalog type "Conference proceedings. fast".
- catalog type "text".