SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion
- Autores
- Qian S. B.; Jiang, L.Q.; Fernandez Lajus, Eduardo Eusebio; Soonthornthum B.; Zhu, L. Y.; Zhao, E. G.; He, J. J.; Liao, W. P.; Wang, J. J.; Liu, L.; Rattanasoon, S.; Aukkaravittayapun, S.; Zhou, X.; Liu, N. P.
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- SDSS J001641-000925 is the first red-dwarf contact binary star with an orbital period of 0.19856 days that is one of the shortest known periods among M-dwarf binary systems. The orbital period was detected to be decreasing rapidly at the rate of dP/dt ~ 8 s/yr. This indicated that SDSS J001641-000925 was undergoing coalescence via a dynamical mass transfer or loss and thus this red-dwarf contact binary is dynamically unstable. To understand the properties of the period change, we monitored the binary system photometrically from September 2, 2011 to October 1, 2014 by using several telescopes in the world and 25 eclipse times were determined. It is discovered that the rapid decrease of the orbital period is not true. This is contrary to the prediction that the system is merging driven by rapid mass transfer or loss. Our preliminary analysis suggests that the Observed-Calculated (O-C) diagram shows a cyclic oscillation with an amplitude of 0.00255 days and a period of 5.7 years. The cyclic variation can be explained by the light-travel time effect via the presence of a cool stellar companion with a mass of M3 sin i′ ~ 0.14M⊙. The orbital separation between the third body and the central binary is about 2.8AU. These results reveal that the rarity of red-dwarf contact binaries could not be explained by rapidly dynamical destruction and the presence of the third body helps to form the red-dwarf contact binary.
Fil: Qian S. B.. Chinese Academy Of Sciences; República de China
Fil: Jiang, L.Q.. Chinese Academy Of Sciences; República de China
Fil: Fernandez Lajus, Eduardo Eusebio. 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
Fil: Soonthornthum B.. National Astronomical Research Insititude of Thailand; Tailandia
Fil: Zhu, L. Y. . Chinese Academy Of Sciences; República de China
Fil: Zhao, E. G. . Chinese Academy Of Sciences; República de China
Fil: He, J. J. . Chinese Academy Of Sciences; República de China
Fil: Liao, W. P. . Chinese Academy Of Sciences; República de China
Fil: Wang, J. J. . Chinese Academy Of Sciences; República de China
Fil: Liu, L.. Chinese Academy Of Sciences; República de China
Fil: Rattanasoon, S.. National Astronomical Research Insititude of Thailand; Tailandia
Fil: Aukkaravittayapun, S.. National Astronomical Research Insititude of Thailand; Tailandia
Fil: Zhou, X.. Chinese Academy Of Sciences; República de China
Fil: Liu, N. P. . Chinese Academy Of Sciences; República de China - Materia
-
Close Binaries
Eclipsing Binaries
Sdss J001641-000925 (Estrella)
Evolution of Stars - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/11157
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SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companionQian S. B.Jiang, L.Q.Fernandez Lajus, Eduardo EusebioSoonthornthum B.Zhu, L. Y. Zhao, E. G. He, J. J. Liao, W. P. Wang, J. J. Liu, L.Rattanasoon, S.Aukkaravittayapun, S.Zhou, X.Liu, N. P. Close BinariesEclipsing BinariesSdss J001641-000925 (Estrella)Evolution of Starshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1SDSS J001641-000925 is the first red-dwarf contact binary star with an orbital period of 0.19856 days that is one of the shortest known periods among M-dwarf binary systems. The orbital period was detected to be decreasing rapidly at the rate of dP/dt ~ 8 s/yr. This indicated that SDSS J001641-000925 was undergoing coalescence via a dynamical mass transfer or loss and thus this red-dwarf contact binary is dynamically unstable. To understand the properties of the period change, we monitored the binary system photometrically from September 2, 2011 to October 1, 2014 by using several telescopes in the world and 25 eclipse times were determined. It is discovered that the rapid decrease of the orbital period is not true. This is contrary to the prediction that the system is merging driven by rapid mass transfer or loss. Our preliminary analysis suggests that the Observed-Calculated (O-C) diagram shows a cyclic oscillation with an amplitude of 0.00255 days and a period of 5.7 years. The cyclic variation can be explained by the light-travel time effect via the presence of a cool stellar companion with a mass of M3 sin i′ ~ 0.14M⊙. The orbital separation between the third body and the central binary is about 2.8AU. These results reveal that the rarity of red-dwarf contact binaries could not be explained by rapidly dynamical destruction and the presence of the third body helps to form the red-dwarf contact binary.Fil: Qian S. B.. Chinese Academy Of Sciences; República de ChinaFil: Jiang, L.Q.. Chinese Academy Of Sciences; República de ChinaFil: Fernandez Lajus, Eduardo Eusebio. 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; ArgentinaFil: Soonthornthum B.. National Astronomical Research Insititude of Thailand; TailandiaFil: Zhu, L. Y. . Chinese Academy Of Sciences; República de ChinaFil: Zhao, E. G. . Chinese Academy Of Sciences; República de ChinaFil: He, J. J. . Chinese Academy Of Sciences; República de ChinaFil: Liao, W. P. . Chinese Academy Of Sciences; República de ChinaFil: Wang, J. J. . Chinese Academy Of Sciences; República de ChinaFil: Liu, L.. Chinese Academy Of Sciences; República de ChinaFil: Rattanasoon, S.. National Astronomical Research Insititude of Thailand; TailandiaFil: Aukkaravittayapun, S.. National Astronomical Research Insititude of Thailand; TailandiaFil: Zhou, X.. Chinese Academy Of Sciences; República de ChinaFil: Liu, N. P. . Chinese Academy Of Sciences; República de ChinaIOP Publishing2015-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/11157Qian S. B.; Jiang, L.Q.; Fernandez Lajus, Eduardo Eusebio; Soonthornthum B.; Zhu, L. Y. ; et al.; SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion; IOP Publishing; Astrophysical Journal Letters; 798; 2; 1-2015; 42-452041-8205enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/798/2/L42info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/798/2/L42/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:27:41Zoai:ri.conicet.gov.ar:11336/11157instacron: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 10:27:41.414CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
title |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
spellingShingle |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion Qian S. B. Close Binaries Eclipsing Binaries Sdss J001641-000925 (Estrella) Evolution of Stars |
title_short |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
title_full |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
title_fullStr |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
title_full_unstemmed |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
title_sort |
SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion |
dc.creator.none.fl_str_mv |
Qian S. B. Jiang, L.Q. Fernandez Lajus, Eduardo Eusebio Soonthornthum B. Zhu, L. Y. Zhao, E. G. He, J. J. Liao, W. P. Wang, J. J. Liu, L. Rattanasoon, S. Aukkaravittayapun, S. Zhou, X. Liu, N. P. |
author |
Qian S. B. |
author_facet |
Qian S. B. Jiang, L.Q. Fernandez Lajus, Eduardo Eusebio Soonthornthum B. Zhu, L. Y. Zhao, E. G. He, J. J. Liao, W. P. Wang, J. J. Liu, L. Rattanasoon, S. Aukkaravittayapun, S. Zhou, X. Liu, N. P. |
author_role |
author |
author2 |
Jiang, L.Q. Fernandez Lajus, Eduardo Eusebio Soonthornthum B. Zhu, L. Y. Zhao, E. G. He, J. J. Liao, W. P. Wang, J. J. Liu, L. Rattanasoon, S. Aukkaravittayapun, S. Zhou, X. Liu, N. P. |
author2_role |
author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Close Binaries Eclipsing Binaries Sdss J001641-000925 (Estrella) Evolution of Stars |
topic |
Close Binaries Eclipsing Binaries Sdss J001641-000925 (Estrella) Evolution of Stars |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
SDSS J001641-000925 is the first red-dwarf contact binary star with an orbital period of 0.19856 days that is one of the shortest known periods among M-dwarf binary systems. The orbital period was detected to be decreasing rapidly at the rate of dP/dt ~ 8 s/yr. This indicated that SDSS J001641-000925 was undergoing coalescence via a dynamical mass transfer or loss and thus this red-dwarf contact binary is dynamically unstable. To understand the properties of the period change, we monitored the binary system photometrically from September 2, 2011 to October 1, 2014 by using several telescopes in the world and 25 eclipse times were determined. It is discovered that the rapid decrease of the orbital period is not true. This is contrary to the prediction that the system is merging driven by rapid mass transfer or loss. Our preliminary analysis suggests that the Observed-Calculated (O-C) diagram shows a cyclic oscillation with an amplitude of 0.00255 days and a period of 5.7 years. The cyclic variation can be explained by the light-travel time effect via the presence of a cool stellar companion with a mass of M3 sin i′ ~ 0.14M⊙. The orbital separation between the third body and the central binary is about 2.8AU. These results reveal that the rarity of red-dwarf contact binaries could not be explained by rapidly dynamical destruction and the presence of the third body helps to form the red-dwarf contact binary. Fil: Qian S. B.. Chinese Academy Of Sciences; República de China Fil: Jiang, L.Q.. Chinese Academy Of Sciences; República de China Fil: Fernandez Lajus, Eduardo Eusebio. 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 Fil: Soonthornthum B.. National Astronomical Research Insititude of Thailand; Tailandia Fil: Zhu, L. Y. . Chinese Academy Of Sciences; República de China Fil: Zhao, E. G. . Chinese Academy Of Sciences; República de China Fil: He, J. J. . Chinese Academy Of Sciences; República de China Fil: Liao, W. P. . Chinese Academy Of Sciences; República de China Fil: Wang, J. J. . Chinese Academy Of Sciences; República de China Fil: Liu, L.. Chinese Academy Of Sciences; República de China Fil: Rattanasoon, S.. National Astronomical Research Insititude of Thailand; Tailandia Fil: Aukkaravittayapun, S.. National Astronomical Research Insititude of Thailand; Tailandia Fil: Zhou, X.. Chinese Academy Of Sciences; República de China Fil: Liu, N. P. . Chinese Academy Of Sciences; República de China |
description |
SDSS J001641-000925 is the first red-dwarf contact binary star with an orbital period of 0.19856 days that is one of the shortest known periods among M-dwarf binary systems. The orbital period was detected to be decreasing rapidly at the rate of dP/dt ~ 8 s/yr. This indicated that SDSS J001641-000925 was undergoing coalescence via a dynamical mass transfer or loss and thus this red-dwarf contact binary is dynamically unstable. To understand the properties of the period change, we monitored the binary system photometrically from September 2, 2011 to October 1, 2014 by using several telescopes in the world and 25 eclipse times were determined. It is discovered that the rapid decrease of the orbital period is not true. This is contrary to the prediction that the system is merging driven by rapid mass transfer or loss. Our preliminary analysis suggests that the Observed-Calculated (O-C) diagram shows a cyclic oscillation with an amplitude of 0.00255 days and a period of 5.7 years. The cyclic variation can be explained by the light-travel time effect via the presence of a cool stellar companion with a mass of M3 sin i′ ~ 0.14M⊙. The orbital separation between the third body and the central binary is about 2.8AU. These results reveal that the rarity of red-dwarf contact binaries could not be explained by rapidly dynamical destruction and the presence of the third body helps to form the red-dwarf contact binary. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-01 |
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/11336/11157 Qian S. B.; Jiang, L.Q.; Fernandez Lajus, Eduardo Eusebio; Soonthornthum B.; Zhu, L. Y. ; et al.; SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion; IOP Publishing; Astrophysical Journal Letters; 798; 2; 1-2015; 42-45 2041-8205 |
url |
http://hdl.handle.net/11336/11157 |
identifier_str_mv |
Qian S. B.; Jiang, L.Q.; Fernandez Lajus, Eduardo Eusebio; Soonthornthum B.; Zhu, L. Y. ; et al.; SDSS J001641-000925: the First Stable Red-dwarf contact binary with a close-in stellar companion; IOP Publishing; Astrophysical Journal Letters; 798; 2; 1-2015; 42-45 2041-8205 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/798/2/L42 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/798/2/L42/meta |
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) |
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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 |