Dataciencia

Colección SciELO Chile

The beta Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members

Indexado

WoS	WOS:000400754000039
Scopus	SCOPUS_ID:85017174979

DOI

10.1051/0004-6361/201629152

Año

2017

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. We provided an extensive catalog of rotation periods together with other relevant basic properties useful to explore a number of open issues, such as the causes of spread of rotation periods among coeval stars, evolution of angular momentum, and lithium-rotation connection.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

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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	Messina, Sergio	Hombre	Istituto Nazionale di Astrofisica - Italia Osservatorio Astrofisico di Catania - Italia INAF - Italia
2	Millward, M.	-	York Creek Observ - Australia York Creek Observatory - Australia
3	Buccino, A. P.	Mujer	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV BUENOS AIRES - Argentina Instituto de Astronomía y Física del Espacio - Argentina Universidad de Buenos Aires - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
4	Zhang, L.	-	Guizhou Univ - China
5	Medhi, B. J.	-	Aryabhatta Res Inst Observat Sci - India Aryabhatta Research Institute of Observational Sciences - India
6	Jofre, E.	Hombre	Observ Astron - Argentina Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
7	Petrucci, R.	Mujer	Observ Astron - Argentina Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
8	Pi, Q.	-	Guizhou Univ - China Guizhou University - China
9	Hambsch, F-J	Hombre	VVS - Bélgica AAVSO - Estados Unidos Vereniging voor Sterrenkunde (VVS) - Bélgica American Association of Variable Star Observers - Estados Unidos
10	Kehusmaa, Petri	Hombre	San Pedro de Atacama Celestial Explorations - Chile Harlingten Atacama Observatory - Chile
11	Harlingten, Caisey	-	San Pedro de Atacama Celestial Explorations - Chile Harlingten Atacama Observatory - Chile
12	Artemenko, S.	-	Res Inst Crimean Astrophys Observ - Ucrania Crimean Astrophysical Observatory RAS - Ucrania
13	MENDEZ-CACERES, NATALIA ANDREA	Hombre	IAU Minor Planet Ctr Code D79 - Australia IAU Minor Planet Center Code D79 - Australia
14	Hentunen, Veli-Pekka	Hombre	Taurus Hill Observ - Finlandia Taurus Hill Observatory - Finlandia
15	Malo, Lison	Mujer	Canada France Hawaii Telescope - Estados Unidos Canada France Hawaii Telescope Corporation - Estados Unidos Télescope Canada-France-Hawaii - Estados Unidos
16	Mauas, P.	Hombre	Comision Nacional de Investigacion Cientifica y Tecnologica - Argentina UNIV BUENOS AIRES - Argentina Instituto de Astronomía y Física del Espacio - Argentina Universidad de Buenos Aires - Argentina Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) - Argentina
17	Monard, Berto	Hombre	Klein Karoo Observ - República de Sudáfrica Klein Karoo Observatory - República de Sudáfrica Kleinkaroo Observatory - República de Sudáfrica
18	Muro Serrano, M.	-	Zeta UMa Observ - España Zeta UMa Observatory - España
19	Naves, Rodrigo	Hombre	Montcabrer Observ - España Observatori Montcabrer - España
20	Santallo, Roland	Hombre	Southern Stars Observ - Francia Southern Stars Observatory - Francia
21	Savuskin, A.	-	Res Inst Crimean Astrophys Observ - Ucrania Crimean Astrophysical Observatory RAS - Ucrania
22	Tan, T. -G.	-	Perth Exoplanet Survey Telescope - Australia

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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
National Science Foundation
National Natural Science Foundation of China (NSFC)
Chinese Academy of Sciences (CAS)
John Templeton Foundation
David and Lucile Packard Fellowship for Science and Engineering
UKs Science and Technology Facilities Council
MIUR (Ministero dell'Istruzione, dell'Universita e della Ricerca)
Directorate for Mathematical and Physical Sciences

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Agradecimientos

Agradecimiento
Research on stellar activity at INAF-Catania Astrophysical Observatory is supported by MIUR (Ministero dell'Istruzione, dell'Universita e della Ricerca). This research has made use of the Simbad database, operated at CDS (Strasbourg, France). We thank the referee Dr. Alexander Scholz for helpful comments. We 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 Queens University Belfast, St. Andrews University, and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UKs Science and Technology Facilities Council. This paper makes use of data from the MEarth Project, which is a collaboration between Harvard University and the Smithsonian Astrophysical Observatory. The MEarth Project acknowledges funding from the David and Lucile Packard Fellowship for Science and Engineering and the National Science Foundation under grants AST-0807690, AST-1109468, AST-1616624 and AST-1004488 (Alan T. Waterman Award), and a grant from the John Templeton Foundation. L.Z. acknowledges the support by the Joint Research Fund in Astronomy (U1431114 and U1631236) under cooperative agreement between the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). This work made use of LAMOST data (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST), which is a National Major Scientific Project built by the Chinese Academy of Sciences.
National Science Foundation under grants AST-0807690, AST-1109468, AST-1616624

Agradecimiento

Research on stellar activity at INAF-Catania Astrophysical Observatory is supported by MIUR (Ministero dell'Istruzione, dell'Universita e della Ricerca). This research has made use of the Simbad database, operated at CDS (Strasbourg, France). We thank the referee Dr. Alexander Scholz for helpful comments. We 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 Queens University Belfast, St. Andrews University, and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UKs Science and Technology Facilities Council. This paper makes use of data from the MEarth Project, which is a collaboration between Harvard University and the Smithsonian Astrophysical Observatory. The MEarth Project acknowledges funding from the David and Lucile Packard Fellowship for Science and Engineering and the National Science Foundation under grants AST-0807690, AST-1109468, AST-1616624 and AST-1004488 (Alan T. Waterman Award), and a grant from the John Templeton Foundation. L.Z. acknowledges the support by the Joint Research Fund in Astronomy (U1431114 and U1631236) under cooperative agreement between the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). This work made use of LAMOST data (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST), which is a National Major Scientific Project built by the Chinese Academy of Sciences.

National Science Foundation under grants AST-0807690, AST-1109468, AST-1616624