![Mass Loss from Stars [electronic resource] : Proceedings of the Second Trieste Colloquium on Astrophysics, 12–17 September, 1968 /](/search/themes/bootstrap3/images/libros.png)
Mass Loss from Stars [electronic resource] : Proceedings of the Second Trieste Colloquium on Astrophysics, 12–17 September, 1968 /
Mass Loss from Stars: A Review -- Session I Mass Loss from Single Stars. Observations -- The Wolf-Rayet Stars and Mass Loss -- Mass Loss from P Cygni -- Rocket Observations of Mass Loss from Hot Stars -- Intrinsic Polarization for Objects with Extended Atmospheres -- Mass Loss from OB Supergiants -- Evidence for Mass Loss from the F-Type Supergiant, 89 Herculis -- A New Outburst of the Shell Star 48 Librae -- Microturbulence in Stellar Atmospheres. Methodic Remark -- Session II Mass Loss from Single Stars. Theories -- Recent Studies of Models for Unstable Stars -- Possibility of Mass Loss in the Red-Giant Stage from H-R Diagrams of Galactic Clusters -- The Colour-Magnitude Distribution of Giants in Open Clusters -- Solar-Wind Model including the Effects of Rotation, Magnetic Fields, and Anisotropic Heat Conduction -- Mass Loss from Coronae and its Effect upon Stellar Rotation -- Coronae around Helium Stars and X-Ray Sources -- Mass Loss from Fast Rotating Stars -- Angular Momentum Considerations and Mass Loss -- Session III Mass Loss from Binary Stars. Observations -- Mass Loss from Close Binaries, 1941–68 -- General Review of Observational Spectroscopic Evidence for Mass Loss in Close Binaries -- Spectroscopic Study of the Eclipsing System R Canis Majoris -- A Gross Secular Expansion of the Primary in RW Persei -- Boss 5481 during the Shell Episode of 1965–67 -- Mass Motions in the System of VV Cephei -- Periods of Eclipsing Novalike Variables -- About the Interpretation of Gaseous Streams in Close Binary Systems -- Mass Exchange in the Binary System AD Herculis obtained from Photometric Observations -- Period Changes of W Ursae Maioris Systems -- Session IV Mass Loss from Close Binaries. Theories -- Mass Exchange in Close Binary Systems with Primary Components of 30 M? -- Evolution of Close Binaries and Origin of Algol-Type Systems -- On the Time-Scale of the Mass Transfer in Close Binaries -- Mass Exchange in Close Binaries of Moderate Mass and Short Periods -- Evolution through Mass Exchange in Close Binary Systems of Total Mass 2.5 M? -- Mass Exchange in Close Binaries of Moderate Period and Mass -- White-Dwarf Production in Binary Systems of Large Separation -- Possible Effects of the Resonance in Close Binaries on their Mass Exchanges -- Some Problems concerning Gas Flows in Close Binary Systems of Dwarf Stars -- Les étoiles doubles, indicatrices d’une perte de masse séculaire des étoiles -- Session V Mass Loss from Unstable Stars -- Infrared Spectra of Nova Delphini 1967 -- Nova Delphini 1967–8 -- Polarization of Nova Delphini 1967 -- Fresh Evidence concerning the Type of Ejection of Novae -- A Mechanism for the Production of Planetary Nebulae -- Photoelectric Observations of CH Cygni during the Explosive Phases of 1967–68 -- Spectroscopic Evidence for Mass Loss from CH Cygni.
| Main Authors: | , |
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| Format: | Texto biblioteca |
| Language: | eng |
| Published: |
Dordrecht : Springer Netherlands,
1969
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| Subjects: | Physics., Observations, Astronomical., Astronomy, Astronomy, Observations and Techniques., |
| Online Access: | http://dx.doi.org/10.1007/978-94-010-3405-0 |
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| Summary: | Mass Loss from Stars: A Review -- Session I Mass Loss from Single Stars. Observations -- The Wolf-Rayet Stars and Mass Loss -- Mass Loss from P Cygni -- Rocket Observations of Mass Loss from Hot Stars -- Intrinsic Polarization for Objects with Extended Atmospheres -- Mass Loss from OB Supergiants -- Evidence for Mass Loss from the F-Type Supergiant, 89 Herculis -- A New Outburst of the Shell Star 48 Librae -- Microturbulence in Stellar Atmospheres. Methodic Remark -- Session II Mass Loss from Single Stars. Theories -- Recent Studies of Models for Unstable Stars -- Possibility of Mass Loss in the Red-Giant Stage from H-R Diagrams of Galactic Clusters -- The Colour-Magnitude Distribution of Giants in Open Clusters -- Solar-Wind Model including the Effects of Rotation, Magnetic Fields, and Anisotropic Heat Conduction -- Mass Loss from Coronae and its Effect upon Stellar Rotation -- Coronae around Helium Stars and X-Ray Sources -- Mass Loss from Fast Rotating Stars -- Angular Momentum Considerations and Mass Loss -- Session III Mass Loss from Binary Stars. Observations -- Mass Loss from Close Binaries, 1941–68 -- General Review of Observational Spectroscopic Evidence for Mass Loss in Close Binaries -- Spectroscopic Study of the Eclipsing System R Canis Majoris -- A Gross Secular Expansion of the Primary in RW Persei -- Boss 5481 during the Shell Episode of 1965–67 -- Mass Motions in the System of VV Cephei -- Periods of Eclipsing Novalike Variables -- About the Interpretation of Gaseous Streams in Close Binary Systems -- Mass Exchange in the Binary System AD Herculis obtained from Photometric Observations -- Period Changes of W Ursae Maioris Systems -- Session IV Mass Loss from Close Binaries. Theories -- Mass Exchange in Close Binary Systems with Primary Components of 30 M? -- Evolution of Close Binaries and Origin of Algol-Type Systems -- On the Time-Scale of the Mass Transfer in Close Binaries -- Mass Exchange in Close Binaries of Moderate Mass and Short Periods -- Evolution through Mass Exchange in Close Binary Systems of Total Mass 2.5 M? -- Mass Exchange in Close Binaries of Moderate Period and Mass -- White-Dwarf Production in Binary Systems of Large Separation -- Possible Effects of the Resonance in Close Binaries on their Mass Exchanges -- Some Problems concerning Gas Flows in Close Binary Systems of Dwarf Stars -- Les étoiles doubles, indicatrices d’une perte de masse séculaire des étoiles -- Session V Mass Loss from Unstable Stars -- Infrared Spectra of Nova Delphini 1967 -- Nova Delphini 1967–8 -- Polarization of Nova Delphini 1967 -- Fresh Evidence concerning the Type of Ejection of Novae -- A Mechanism for the Production of Planetary Nebulae -- Photoelectric Observations of CH Cygni during the Explosive Phases of 1967–68 -- Spectroscopic Evidence for Mass Loss from CH Cygni. |
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