Dataciencia

Colección SciELO Chile

Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue

Indexado

WoS

WOS:000341185300005

DOI

10.1051/0004-63615201220985

Año

2014

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions, AK For is the brightest system among the known eclipsing binaries with K- or M-type stars, Its orbital period is one of the longest, and its rotational velocities is one of the lowest, which allows us to obtain very precise radial velocity measurements. The precision in physical parameters that we obtained places AK For among the binaries with the best mass measurements in the literature It also fills the gap in our knowledge of stars in the range of 0.5-0.8 M-circle dot and between short and long-period systems. All this makes AK For a unique benchmark for understanding the properties of low mass stars.

Revista

Revista	ISSN
Astronomy & Astrophysics	1432-0746

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Helminiak, K. G.	Hombre	Pontificia Universidad Católica de Chile - Chile Nicolaus Copernicus Astron Ctr - Polonia Natl Astron Observ Japan - Estados Unidos
2	BRAHM-SCOTT, RAFAEL ANDRES	Hombre	Pontificia Universidad Católica de Chile - Chile
3	Ratajczak, M.	Mujer	Nicolaus Copernicus Astron Ctr - Polonia
4	Espinoza, Nestor	Hombre	Pontificia Universidad Católica de Chile - Chile
5	JORDAN-COLZANI, ANDRES CRISTOBAL	Hombre	Pontificia Universidad Católica de Chile - Chile Instituto Milenio de Astrofísica - Chile
6	Konacki, M.	Hombre	Nicolaus Copernicus Astron Ctr - Polonia Adam Mickiewicz Univ - Polonia
7	Rabus, M.	-	Pontificia Universidad Católica de Chile - Chile Max Planck Inst Astron - Alemania

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 22.22 %
Citas No-identificadas: 77.78 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 22.22 %
Citas No-identificadas: 77.78 %

Financiamiento

Fuente
FONDECYT
CONICYT-PCHA/Doctorado Nacional
European Research Council
Polish National Science Center
Proyecto FONDECYT
BASAL CATA
Ministry of Science and Higher Education
UK's Science and Technology Facilities Council
National Astronomical Observatory of Japan
Foundation for Polish Science
National Aeronautics and Space Administration and the National Science Foundation

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Agradecimientos

Agradecimiento
We would like to thank Dr Johannnes And for the discussion and valuable comments that helped us improve our manuscript and the staff of the La Silla and Geneva absent:atones, especially G. Lambert and D. Naef for their hospitality and help during the observations. K.G.H. acknowledges support provided by the Proyecto FONDECYT Postdoctoral No. 3120153, the Polish National Science Center grant 2011/03/N/8T9/01819, and the National Astronomical Observatory of Japan as Subaru Astronomical Research R.B. and N.E. are supported by CONICYT-PCHA/Doctorado Nacional. M. Ratajezak is supported by the Polish National Science Center through grant 2011/01/N/ST9/02209. Ad. acknowledges support from FONDECYT project 1130857, BASAL CATA PEB-06. and grant IC120009 awarded to the Millennium Institute of Astrophysics, MAS, by the Millennium Science Initiative of the Chilean Ministry of Economy, Development, and Tourism. M.K. is supported by the European Research Council Starting Grant. the Polish National Science Center through grant 5813/B/H03/2011/40. the Ministry of Science and Higher Education through grant W103/ERC/2011 and the Foundation for Polish Science through grant "Ideas for Poland". M. Rabus acknowledges support from FONDECYT postdoctoral fellowship No. 3120097. Be have used data from the WASP public archive in this research, The WASP consortium comprises of the University of Cambridge, Keele University, University of Leicester, The Open University. The Queen's University Belfast, St. Andrews University and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UK's Science and Technology Facilities Council. This publication makes use of data products from the Two Micron All Sky Survey which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.

Agradecimiento

We would like to thank Dr Johannnes And for the discussion and valuable comments that helped us improve our manuscript and the staff of the La Silla and Geneva absent:atones, especially G. Lambert and D. Naef for their hospitality and help during the observations. K.G.H. acknowledges support provided by the Proyecto FONDECYT Postdoctoral No. 3120153, the Polish National Science Center grant 2011/03/N/8T9/01819, and the National Astronomical Observatory of Japan as Subaru Astronomical Research R.B. and N.E. are supported by CONICYT-PCHA/Doctorado Nacional. M. Ratajezak is supported by the Polish National Science Center through grant 2011/01/N/ST9/02209. Ad. acknowledges support from FONDECYT project 1130857, BASAL CATA PEB-06. and grant IC120009 awarded to the Millennium Institute of Astrophysics, MAS, by the Millennium Science Initiative of the Chilean Ministry of Economy, Development, and Tourism. M.K. is supported by the European Research Council Starting Grant. the Polish National Science Center through grant 5813/B/H03/2011/40. the Ministry of Science and Higher Education through grant W103/ERC/2011 and the Foundation for Polish Science through grant "Ideas for Poland". M. Rabus acknowledges support from FONDECYT postdoctoral fellowship No. 3120097. Be have used data from the WASP public archive in this research, The WASP consortium comprises of the University of Cambridge, Keele University, University of Leicester, The Open University. The Queen's University Belfast, St. Andrews University and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UK's Science and Technology Facilities Council. This publication makes use of data products from the Two Micron All Sky Survey which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.

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Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección