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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...
Autores principales: | , , |
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Lenguaje: | eng |
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Springer
2008
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Acceso en línea: | https://dx.doi.org/10.1007/978-3-540-74745-1 http://cds.cern.ch/record/1338685 |
_version_ | 1780921903569960960 |
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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. |
id | cern-1338685 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
publisher | Springer |
record_format | invenio |
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 |