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Multiple Stars Across the H-R Diagram

Stars show a marked tendency to be in systems of different multiplicity, ranging from simple binaries and triples to globular clusters with several 10,000's of stars. The formation and evolution of multiple systems remains a challenging part of astrophysics, and the contributions in this book r...

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Detalles Bibliográficos
Autores principales: Hubrig, Swetlana, Petr-Gotzens, Monika, Tokovinin, Andrei
Lenguaje:eng
Publicado: Springer 2008
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-540-74745-1
http://cds.cern.ch/record/1338685
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author Hubrig, Swetlana
Petr-Gotzens, Monika
Tokovinin, Andrei
author_facet Hubrig, Swetlana
Petr-Gotzens, Monika
Tokovinin, Andrei
author_sort Hubrig, Swetlana
collection CERN
description Stars show a marked tendency to be in systems of different multiplicity, ranging from simple binaries and triples to globular clusters with several 10,000's of stars. The formation and evolution of multiple systems remains a challenging part of astrophysics, and the contributions in this book report on the significant progress that had been made in this research field in the last years. The reader will find a variety of research topics addressed, such as the dynamical evolution in multiple stars, the effects of the environment on multiple system parameters, stellar evolution within multiple stars, multiplicity of massive stars, pre-main sequence and intermediate mass stars, multiplicity of low-mass stars from embedded protostars to open clusters, and brown dwarfs and extrasolar planets in multiples. This book presents the proceedings of the ESO Workshop on Multiple Stars across the H-R Diagram held in the summer of 2005.
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spelling cern-13386852021-04-25T17:14:46Zdoi:10.1007/978-3-540-74745-1http://cds.cern.ch/record/1338685engHubrig, SwetlanaPetr-Gotzens, MonikaTokovinin, AndreiMultiple Stars Across the H-R DiagramAstrophysics and AstronomyStars show a marked tendency to be in systems of different multiplicity, ranging from simple binaries and triples to globular clusters with several 10,000's of stars. The formation and evolution of multiple systems remains a challenging part of astrophysics, and the contributions in this book report on the significant progress that had been made in this research field in the last years. The reader will find a variety of research topics addressed, such as the dynamical evolution in multiple stars, the effects of the environment on multiple system parameters, stellar evolution within multiple stars, multiplicity of massive stars, pre-main sequence and intermediate mass stars, multiplicity of low-mass stars from embedded protostars to open clusters, and brown dwarfs and extrasolar planets in multiples. This book presents the proceedings of the ESO Workshop on Multiple Stars across the H-R Diagram held in the summer of 2005.Springeroai:cds.cern.ch:13386852008
spellingShingle Astrophysics and Astronomy
Hubrig, Swetlana
Petr-Gotzens, Monika
Tokovinin, Andrei
Multiple Stars Across the H-R Diagram
title Multiple Stars Across the H-R Diagram
title_full Multiple Stars Across the H-R Diagram
title_fullStr Multiple Stars Across the H-R Diagram
title_full_unstemmed Multiple Stars Across the H-R Diagram
title_short Multiple Stars Across the H-R Diagram
title_sort multiple stars across the h-r diagram
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1007/978-3-540-74745-1
http://cds.cern.ch/record/1338685
work_keys_str_mv AT hubrigswetlana multiplestarsacrossthehrdiagram
AT petrgotzensmonika multiplestarsacrossthehrdiagram
AT tokovininandrei multiplestarsacrossthehrdiagram