Lithium production in the merging of white dwarf stars
- Autores
- Longland, Richard; Loren Aguilar, P.; José, Jordi; García Berro, E.; Althaus, Leandro Gabriel
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The origin of R Coronae Borealis stars has been elusive for over 200 years. Currently, two theories for their formation have been presented. These are the final flash scenario, in which a dying asymptotic giant branch star throws off its atmosphere to reveal the hydrogen poor, heavily processed material underneath, and the double degenerate scenario, in which two white dwarfs merge to produce a new star with renewed vigour. Some theories predict that the temperatures reached during the latter scenario would destroy any lithium originally present in the white dwarfs. The observed lithium content of some R Coronae Borealis stars, therefore, is often interpreted as an indication that the final flash scenario best describes their formation. In this paper, we show that lithium production can, indeed, occur in the merging of a helium white dwarf with a carbon-oxygen white dwarf if their chemical composition, particularly that of 3He, is fully considered. The production mechanism is described in detail, and the sensitivity of lithium production to the merger environment is investigated. Nucleosynthesis post-processing calculations of smoothed-particle hydrodynamics (SPH) tracer particles are performed to show that any lithium produced in these environments will be concentrated towards the cloud of material surrounding the R CrB star. Measurements of the lithium content of these clouds would, therefore, provide a valuable insight into the formation mechanism of R CrB stars.
Fil: Longland, Richard. Institut d’Estudis Espacials de Catalunya; España
Fil: Loren Aguilar, P.. Institut d’Estudis Espacials de Catalunya; España. Universidad Politecnica de Catalunya; España
Fil: José, Jordi. Universitat Oberta de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina - Materia
-
Nuclear reactions
Abundances
White dwarfs stars
AGB and post-AGB
Evolution of stars
Nucleosynthesis - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/8291
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Lithium production in the merging of white dwarf starsLongland, RichardLoren Aguilar, P.José, JordiGarcía Berro, E.Althaus, Leandro GabrielNuclear reactionsAbundancesWhite dwarfs starsAGB and post-AGBEvolution of starsNucleosynthesishttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The origin of R Coronae Borealis stars has been elusive for over 200 years. Currently, two theories for their formation have been presented. These are the final flash scenario, in which a dying asymptotic giant branch star throws off its atmosphere to reveal the hydrogen poor, heavily processed material underneath, and the double degenerate scenario, in which two white dwarfs merge to produce a new star with renewed vigour. Some theories predict that the temperatures reached during the latter scenario would destroy any lithium originally present in the white dwarfs. The observed lithium content of some R Coronae Borealis stars, therefore, is often interpreted as an indication that the final flash scenario best describes their formation. In this paper, we show that lithium production can, indeed, occur in the merging of a helium white dwarf with a carbon-oxygen white dwarf if their chemical composition, particularly that of 3He, is fully considered. The production mechanism is described in detail, and the sensitivity of lithium production to the merger environment is investigated. Nucleosynthesis post-processing calculations of smoothed-particle hydrodynamics (SPH) tracer particles are performed to show that any lithium produced in these environments will be concentrated towards the cloud of material surrounding the R CrB star. Measurements of the lithium content of these clouds would, therefore, provide a valuable insight into the formation mechanism of R CrB stars.Fil: Longland, Richard. Institut d’Estudis Espacials de Catalunya; EspañaFil: Loren Aguilar, P.. Institut d’Estudis Espacials de Catalunya; España. Universidad Politecnica de Catalunya; EspañaFil: José, Jordi. Universitat Oberta de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaEdp Sciences2012-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/8291Longland, Richard; Loren Aguilar, P.; José, Jordi; García Berro, E.; Althaus, Leandro Gabriel; Lithium production in the merging of white dwarf stars; Edp Sciences; Astronomy And Astrophysics; 542; A117; 6-2012; 117-1230004-6361enginfo:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2012/06/aa19289-12/aa19289-12.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201219289info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1205.2538v1info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:50Zoai:ri.conicet.gov.ar:11336/8291instacron: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 09:33:51.077CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Lithium production in the merging of white dwarf stars |
title |
Lithium production in the merging of white dwarf stars |
spellingShingle |
Lithium production in the merging of white dwarf stars Longland, Richard Nuclear reactions Abundances White dwarfs stars AGB and post-AGB Evolution of stars Nucleosynthesis |
title_short |
Lithium production in the merging of white dwarf stars |
title_full |
Lithium production in the merging of white dwarf stars |
title_fullStr |
Lithium production in the merging of white dwarf stars |
title_full_unstemmed |
Lithium production in the merging of white dwarf stars |
title_sort |
Lithium production in the merging of white dwarf stars |
dc.creator.none.fl_str_mv |
Longland, Richard Loren Aguilar, P. José, Jordi García Berro, E. Althaus, Leandro Gabriel |
author |
Longland, Richard |
author_facet |
Longland, Richard Loren Aguilar, P. José, Jordi García Berro, E. Althaus, Leandro Gabriel |
author_role |
author |
author2 |
Loren Aguilar, P. José, Jordi García Berro, E. Althaus, Leandro Gabriel |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Nuclear reactions Abundances White dwarfs stars AGB and post-AGB Evolution of stars Nucleosynthesis |
topic |
Nuclear reactions Abundances White dwarfs stars AGB and post-AGB Evolution of stars Nucleosynthesis |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The origin of R Coronae Borealis stars has been elusive for over 200 years. Currently, two theories for their formation have been presented. These are the final flash scenario, in which a dying asymptotic giant branch star throws off its atmosphere to reveal the hydrogen poor, heavily processed material underneath, and the double degenerate scenario, in which two white dwarfs merge to produce a new star with renewed vigour. Some theories predict that the temperatures reached during the latter scenario would destroy any lithium originally present in the white dwarfs. The observed lithium content of some R Coronae Borealis stars, therefore, is often interpreted as an indication that the final flash scenario best describes their formation. In this paper, we show that lithium production can, indeed, occur in the merging of a helium white dwarf with a carbon-oxygen white dwarf if their chemical composition, particularly that of 3He, is fully considered. The production mechanism is described in detail, and the sensitivity of lithium production to the merger environment is investigated. Nucleosynthesis post-processing calculations of smoothed-particle hydrodynamics (SPH) tracer particles are performed to show that any lithium produced in these environments will be concentrated towards the cloud of material surrounding the R CrB star. Measurements of the lithium content of these clouds would, therefore, provide a valuable insight into the formation mechanism of R CrB stars. Fil: Longland, Richard. Institut d’Estudis Espacials de Catalunya; España Fil: Loren Aguilar, P.. Institut d’Estudis Espacials de Catalunya; España. Universidad Politecnica de Catalunya; España Fil: José, Jordi. Universitat Oberta de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: García Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina |
description |
The origin of R Coronae Borealis stars has been elusive for over 200 years. Currently, two theories for their formation have been presented. These are the final flash scenario, in which a dying asymptotic giant branch star throws off its atmosphere to reveal the hydrogen poor, heavily processed material underneath, and the double degenerate scenario, in which two white dwarfs merge to produce a new star with renewed vigour. Some theories predict that the temperatures reached during the latter scenario would destroy any lithium originally present in the white dwarfs. The observed lithium content of some R Coronae Borealis stars, therefore, is often interpreted as an indication that the final flash scenario best describes their formation. In this paper, we show that lithium production can, indeed, occur in the merging of a helium white dwarf with a carbon-oxygen white dwarf if their chemical composition, particularly that of 3He, is fully considered. The production mechanism is described in detail, and the sensitivity of lithium production to the merger environment is investigated. Nucleosynthesis post-processing calculations of smoothed-particle hydrodynamics (SPH) tracer particles are performed to show that any lithium produced in these environments will be concentrated towards the cloud of material surrounding the R CrB star. Measurements of the lithium content of these clouds would, therefore, provide a valuable insight into the formation mechanism of R CrB stars. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-06 |
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/11336/8291 Longland, Richard; Loren Aguilar, P.; José, Jordi; García Berro, E.; Althaus, Leandro Gabriel; Lithium production in the merging of white dwarf stars; Edp Sciences; Astronomy And Astrophysics; 542; A117; 6-2012; 117-123 0004-6361 |
url |
http://hdl.handle.net/11336/8291 |
identifier_str_mv |
Longland, Richard; Loren Aguilar, P.; José, Jordi; García Berro, E.; Althaus, Leandro Gabriel; Lithium production in the merging of white dwarf stars; Edp Sciences; Astronomy And Astrophysics; 542; A117; 6-2012; 117-123 0004-6361 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2012/06/aa19289-12/aa19289-12.html info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201219289 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1205.2538v1 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Edp Sciences |
publisher.none.fl_str_mv |
Edp Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |