Dataciencia

Colección SciELO Chile

Young open clusters in the Galactic star forming region NGC 6357

Indexado

WoS	WOS:000346901300044
Scopus	SCOPUS_ID:84919779790

DOI

10.1051/0004-6361/201424388

Año

2015

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. Our findings provide some new insight into how young stellar populations and massive stars emerge, and evolve in the first few Myr after birth, from a giant molecular cloud complex.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

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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	Massi, F.	-	Osserv Astrofis Arcetri - Italia Osservatorio Astrofisico Di Arcetri - Italia
2	Giannetti, A.	-	Ist Radioastron - Italia Italian ALMA Reg Ctr - Italia
3	Di Carlo, E.	Mujer	Osservatorio Astron Collurania Teramo - Italia Osservatorio Astronomico di Collurania Vincenzo Cerulli - Italia
4	Brand, J.	-	Ist Radioastron - Italia Italian ALMA Reg Ctr - Italia
5	Beltran, Maria T.	Mujer	Osserv Astrofis Arcetri - Italia Osservatorio Astrofisico Di Arcetri - Italia
6	Marconi, G.	-	ESO - Chile

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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: 6.67 %
Citas No-identificadas: 93.33 %

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

Citas Identificadas: 6.67 %
Citas No-identificadas: 93.33 %

Financiamiento

Fuente
National Science Foundation
NASA
National Aeronautics and Space Administration
US Government
PRIN INAF

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. It is also partially based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program # 9091 (P.I. Jeff Hester). 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. The Digitized Sky Survey (DSS) was produced at the Space Telescope Science Institute under US Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. F.M. and E.D.C. acknowledge partial funding by the PRIN INAF 2009 grant CRA 1.06.12.10 ("Formation and early evolution of massive star clusters", P.I.R. Gratton). EDC is also grateful for financial support from PRIN INAF 2011 ("Multiple Populations in Globular Clusters: their role in the Galaxy assembly", P.I.: E. Carretta).
This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. It is also partially based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program # 9091 (P.I. Jeff Hester). 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. The Digitized Sky Survey (DSS) was produced at the Space Telescope Science Institute under US Government grant NAG W–2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. F.M. and E.D.C. acknowledge partial funding by the PRIN INAF 2009 grant CRA 1.06.12.10 (“Formation and early evolution of massive star clusters”, P.I. R. Gratton). EDC is also grateful for financial support from PRIN INAF 2011 (“Multiple Populations in Globular Clusters: their role in the Galaxy assembly”, P.I.: E. Carretta).

Agradecimiento

This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. It is also partially based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program # 9091 (P.I. Jeff Hester). 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. The Digitized Sky Survey (DSS) was produced at the Space Telescope Science Institute under US Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. F.M. and E.D.C. acknowledge partial funding by the PRIN INAF 2009 grant CRA 1.06.12.10 ("Formation and early evolution of massive star clusters", P.I.R. Gratton). EDC is also grateful for financial support from PRIN INAF 2011 ("Multiple Populations in Globular Clusters: their role in the Galaxy assembly", P.I.: E. Carretta).

This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. It is also partially based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program # 9091 (P.I. Jeff Hester). 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. The Digitized Sky Survey (DSS) was produced at the Space Telescope Science Institute under US Government grant NAG W–2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. F.M. and E.D.C. acknowledge partial funding by the PRIN INAF 2009 grant CRA 1.06.12.10 (“Formation and early evolution of massive star clusters”, P.I. R. Gratton). EDC is also grateful for financial support from PRIN INAF 2011 (“Multiple Populations in Globular Clusters: their role in the Galaxy assembly”, P.I.: E. Carretta).

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección