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A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy

Indexado

WoS	WOS:000503239600003
Scopus	SCOPUS_ID:85092064921

DOI

10.1051/0004-6361/201936431

Año

2019

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Results. We obtained a mean metallicity of [Fe/H] approximate to 1.10 +/- 0.15, a heliocentric radial velocity of v(r)(h) = 58.1 +/- 1.1 km s(-1), and a magnesium-to-iron [Mg/Fe] = 0.27 +/- 0.03. The metallicity-derived character of Terzan 9 sets it among the family of the moderately metal-poor Blue Horizontal Branch clusters HP 1, NGC 6558, and NGC 6522.

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	Ernandes, H.	Hombre	UNIV SAO PAULO - Brasil Royal Observ - Reino Unido UNIV EDINBURGH - Reino Unido Universidade de São Paulo - Brasil Royal Observatory - Reino Unido The University of Edinburgh - Reino Unido
2	Dias, B.	Hombre	ESO - Chile Universidad Nacional Andrés Bello - Chile European Southern Observatory Santiago - Chile
3	Barbuy, Beatriz	Mujer	UNIV SAO PAULO - Brasil Universidade de São Paulo - Brasil
4	Kamann, Sebastian	Hombre	Liverpool John Moores Univ - Reino Unido Liverpool John Moores University - Reino Unido
5	Ortolani, S.	Hombre	Univ Padua - Italia Istituto Nazionale di Astrofisica - Italia Università degli Studi di Padova - Italia Osservatorio Astronomico di Padova - Italia
6	Cantelli, E.	-	UNIV SAO PAULO - Brasil Universidade de São Paulo - Brasil
7	Bonatto, C. J.	Hombre	Univ Fed Rio Grande do Sul - Brasil Universidade Federal do Rio Grande do Sul - Brasil
8	Rossi, L.	-	Swinburne Univ Technol - Australia

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Financiamiento

Fuente
CAPES
CNPq
FAPESP
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Fundação de Amparo à Pesquisa do Estado de São Paulo
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

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Agradecimientos

Agradecimiento
We are grateful to David Katz for helpful comments on the Etoile code, and to Angeles Perez-Villegas for help with the proper motion and orbital information. HE, BB, EB and EC acknowledge partial financial support, grants and fellowships from FAPESP, CNPq and CAPES - Finance code 001. HE and EC are grateful for their visit to ESO in Santiago, within ESO's o ffice for science programme, under supervision of B. Dias.
Acknowledgements. We are grateful to David Katz for helpful comments on the Etoile code, and to Angeles Pérez-Villegas for help with the proper motion and orbital information. HE, BB, EB and EC acknowledge partial financial support, grants and fellowships from FAPESP, CNPq and CAPES – Finance code 001.

Agradecimiento

We are grateful to David Katz for helpful comments on the Etoile code, and to Angeles Perez-Villegas for help with the proper motion and orbital information. HE, BB, EB and EC acknowledge partial financial support, grants and fellowships from FAPESP, CNPq and CAPES - Finance code 001. HE and EC are grateful for their visit to ESO in Santiago, within ESO's o ffice for science programme, under supervision of B. Dias.

Acknowledgements. We are grateful to David Katz for helpful comments on the Etoile code, and to Angeles Pérez-Villegas for help with the proper motion and orbital information. HE, BB, EB and EC acknowledge partial financial support, grants and fellowships from FAPESP, CNPq and CAPES – Finance code 001.