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Evolution of Massive Stars: A Confrontation between Theory and Observation - Tapa dura

 
9780792327998: Evolution of Massive Stars: A Confrontation between Theory and Observation
Tapa dura
ISBN 10: 0792327993 ISBN 13: 9780792327998
Editorial: Springer, 1994

Sinopsis

Massive stars: setting the stage.- I. Number and Distribution of Massive Stars.- The massive star distribution in the Galaxy and the Magellanic Clouds.- Massive star distribution in external galaxies and starburst region.- Dissection of 30 Doradus and a discussion of the Magellanic Cloud OB-associations.- Blue and red supergiants and the age structure of the NGC 330 region.- Stars in young clusters in the Magellanic Clouds.- The population of massive stars in R136 from HST/FOC UV observations.- Spectral synthesis of spectral populations using Balmer lines.- The stellar content of the Orion OB1 association.- II. Massive Star Atmospheres and Stellar Winds.- Observations of the atmospheres and winds of O-stars, LBV’s and Wolf-Rayet stars.- Radiation driven winds of hot stars: theory of O-star atmospheres as a spectral tool.- The chemical composition of B-supergiant atmospheres.- Intrinsic parameters of massive OB-stars.- Line blanketing by iron group elements in non-LTE model atmospheres of hot stars.- A comparison between observed and predicted mass loss rates and wind momentum of O stars.- LTE and NLTE abundances in A supergiants: a test of their evolutionary status.- A spectroscopic analysis of B-stars in the SMC cluster NGC 330.- Hydrodynamic atmosphere models for hot luminous stars II. Method and improvements over unified models.- Hubble space telescope spectroscopy of massive hot stars in the Magellanic Clouds and M31.- Stellar winds of massive stars in M31.- O-star winds in the Magellanic Clouds and the Milky Way.- On the relation between the mass loss rate and the stellar parameters of OB-type stars.- Wind asymmetries in massive stars.- NLTE analysis of hot binaries.- Effective temperatures and surface gravities of early type stars.- The atmospheric composition, extinction and luminosity of the LBV star R71.- The variability of Eta Car: a tool for the LBV phenomenon.- The nature of the luminous blue variable AG Car.- The evolutionary status of Eta Car based on historical and modern optical and infrared photometry.- The gradual acceleration of the outflow of VX Sagittari; a stellar evolution effect?.- The complex H-alpha profile of the hypergiant HR 8752 during 1970-1992.- Spectral analysis of Wolf-Rayet stars: theory, results, conclusions.- Line-blanketed non-LTE atmosphere models for Wolf-Rayet stars.- The fundamental parameters of the central stars of eight WR ring nebulae.- Tailored analysis of 24 galactic WN stars.- Oxygen and carbon abundances for the WO stars.- HD190918: arbiter between models for Wolf-Rayet stars.- III. Structure and Evolution of Massive Srars.- Structure and evolution of massive stars: mixing processes and stellar evolution.- Overshooting from convective cores: theory and numerical simulation.- Massive close binaries. observational characteristics.- Doppler tomography of O-type binaries; the physical properties of seven systems.- Evolution of massive close binaries.- Massive single star evolution: comparison with observations.- Presupernova evolution of the most massive stars.- Properties of massive star evolution.- Nucleosynthesis in massive stars.- Results of evolutionary computations of primaries of close binaries with different initial composition.- The mass and helium discrepancy in massive stars: the case Vela X-1.- On the evolution of secondary components in massive close binary systems.- Double-zone model with diffusive mixing and the mass and helium discrepancies in OB stars.- The impact of semi-convection and overshooting on the surface abundances in massive stars.- Improved bolometric corrections for WR stars.- Wolf-Rayet stars in starbursts.- A study of the SMC cluster NGC330.- The evolution of massive stars to explosion.- SN1987A and SN1993J: testing stellar evolution theory.- Chemical and photometric evolution of elliptical galaxies.- A model for the chemical evolution of the solar neighborhood using metallicity dependent yields.- Poster list.- Summary.

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Reseña del editor

This book presents a complete overview of what we know -- and would like to know -- about the evolution and structure of massive stars. The spectra of early type stars are produced by elaborate model atmospheres enveloping the internal structure self-consistently. The book is valuable for research on the evolution, structure and atmospheres of massive stars. Astrophysics courses at university level should use the book to get acquainted with the most recent observational data, modeling of the internal and atmospheric structure, and the refined development of single and binary evolution scenarios of massive stars.

Reseña del editor

This book presents a complete overview of what we know, and would like to know, about the evolution and structure of massive stars. The spectra of early-type stars are produced by elaborate model atmospheres enveloping the internal structure. The book should be of value to researchers into the evolution, structure and atmospheres of massive stars. The book is also appropriate for astrophysics courses at university level, where it can be used to get acquainted with the most recent observational data, modelling of the internal and atmospheric structure, and the refined development of single and binary evolution scenarios of massive stars.

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Editorial
Springer
Año de publicación
1994
Idioma
Inglés
ISBN 10 
0792327993
ISBN 13 
9780792327998
Encuadernación
Tapa dura
Número de páginas
504
Editor
De Loore C., Vanbeveren D., Van Rensbergen W.
Contacto del fabricante
Springer Nature Customer Service Center GmbH
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