Analytical solutions for radiation-driven winds in massive stars: I. the fast regime

Autores
Araya, I.; Curé, M.; Cidale, Lydia Sonia
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of differential equations in which the radiation field and the hydrodynamics are strongly coupled. The use of an analytical expression to represent the radiation force and the solution of the equation of motion has many advantages over numerical integrations. Therefore, in this work, we present an analytical expression as a solution of the equation of motion for radiation-driven winds in terms of the force multiplier parameters. This analytical expression is obtained by employing the line acceleration expression given by Villata and the methodology proposed by Muller & Vink. ¨ On the other hand, we find useful relationships to determine the parameters for the line acceleration given by Muller & Vink in terms of the force multiplier parameters.
Fil: Araya, I.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Curé, M.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; Chile
Fil: Cidale, Lydia Sonia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina
Materia
Hydrodynamics
Early-Type Star
Star Winds
Star Mass-Loss
Star Outflows
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/10872
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/10872
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Analytical solutions for radiation-driven winds in massive stars: I. the fast regimeAraya, I.Curé, M.Cidale, Lydia SoniaHydrodynamicsEarly-Type StarStar WindsStar Mass-LossStar Outflowshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of differential equations in which the radiation field and the hydrodynamics are strongly coupled. The use of an analytical expression to represent the radiation force and the solution of the equation of motion has many advantages over numerical integrations. Therefore, in this work, we present an analytical expression as a solution of the equation of motion for radiation-driven winds in terms of the force multiplier parameters. This analytical expression is obtained by employing the line acceleration expression given by Villata and the methodology proposed by Muller & Vink. ¨ On the other hand, we find useful relationships to determine the parameters for the line acceleration given by Muller & Vink in terms of the force multiplier parameters.Fil: Araya, I.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Curé, M.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; ChileFil: Cidale, Lydia Sonia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; ArgentinaIop Publishing2014-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10872Araya, I.; Curé, M.; Cidale, Lydia Sonia; Analytical solutions for radiation-driven winds in massive stars: I. the fast regime; Iop Publishing; Astrophysical Journal; 795; 1; 10-2014; 81-870004-637X1538-4357enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/795/1/81info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/795/1/81/meta;jsessionid=F026C4EC90C24064BDCE605BAAB4FD12.c1.iopscience.cld.iop.orginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1411.0751info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:54:37Zoai:ri.conicet.gov.ar:11336/10872instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:54:37.481CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
title Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
spellingShingle Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
Araya, I.
Hydrodynamics
Early-Type Star
Star Winds
Star Mass-Loss
Star Outflows
title_short Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
title_full Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
title_fullStr Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
title_full_unstemmed Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
title_sort Analytical solutions for radiation-driven winds in massive stars: I. the fast regime
dc.creator.none.fl_str_mv Araya, I.
Curé, M.
Cidale, Lydia Sonia
author Araya, I.
author_facet Araya, I.
Curé, M.
Cidale, Lydia Sonia
author_role author
author2 Curé, M.
Cidale, Lydia Sonia
author2_role author
author
dc.subject.none.fl_str_mv Hydrodynamics
Early-Type Star
Star Winds
Star Mass-Loss
Star Outflows
topic Hydrodynamics
Early-Type Star
Star Winds
Star Mass-Loss
Star Outflows
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of differential equations in which the radiation field and the hydrodynamics are strongly coupled. The use of an analytical expression to represent the radiation force and the solution of the equation of motion has many advantages over numerical integrations. Therefore, in this work, we present an analytical expression as a solution of the equation of motion for radiation-driven winds in terms of the force multiplier parameters. This analytical expression is obtained by employing the line acceleration expression given by Villata and the methodology proposed by Muller & Vink. ¨ On the other hand, we find useful relationships to determine the parameters for the line acceleration given by Muller & Vink in terms of the force multiplier parameters.
Fil: Araya, I.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Curé, M.. Universidad de Valparaíso. Facultad de Ciencias. Instituto de Física y Astronomía; Chile
Fil: Cidale, Lydia Sonia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina
description Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of differential equations in which the radiation field and the hydrodynamics are strongly coupled. The use of an analytical expression to represent the radiation force and the solution of the equation of motion has many advantages over numerical integrations. Therefore, in this work, we present an analytical expression as a solution of the equation of motion for radiation-driven winds in terms of the force multiplier parameters. This analytical expression is obtained by employing the line acceleration expression given by Villata and the methodology proposed by Muller & Vink. ¨ On the other hand, we find useful relationships to determine the parameters for the line acceleration given by Muller & Vink in terms of the force multiplier parameters.
publishDate 2014
dc.date.none.fl_str_mv 2014-10
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/10872
Araya, I.; Curé, M.; Cidale, Lydia Sonia; Analytical solutions for radiation-driven winds in massive stars: I. the fast regime; Iop Publishing; Astrophysical Journal; 795; 1; 10-2014; 81-87
0004-637X
1538-4357
url http://hdl.handle.net/11336/10872
identifier_str_mv Araya, I.; Curé, M.; Cidale, Lydia Sonia; Analytical solutions for radiation-driven winds in massive stars: I. the fast regime; Iop Publishing; Astrophysical Journal; 795; 1; 10-2014; 81-87
0004-637X
1538-4357
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/795/1/81
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/795/1/81/meta;jsessionid=F026C4EC90C24064BDCE605BAAB4FD12.c1.iopscience.cld.iop.org
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1411.0751
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing
publisher.none.fl_str_mv Iop Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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