VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge
- Autores
- McDonald, I.; Zijlstra, A. A.; Sloan, G. C.; Kerins, E. J.; Lagadec, E.; Minniti, Dante; Santucho, María Victoria; Gurovich, Sebastian; Dominguez Romero, Mariano Javier de Leon
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the deepest near-infrared (ZJKs) photometry yet obtained of the Sagittarius dwarf spheroidal (Sgr dSph), using Visible and Infrared Survey Telescope for Astronomy (VISTA) to survey 11 square degrees centred on its core. We list locations and ZJKs-band magnitudes for over 2.9 million sources in the field. We discuss the isolation of the Sgr dSph from the foreground and Galactic Bulge populations, identify the Sgr dSph's horizontal branch in the near-infrared for the first time and map the density of the galaxy's stars. We present isochrones for the Sgr dSph and Bulge populations. These are consistent with the previously reported properties of the Sgr dSph core: namely that it is dominated by a population between [Fe/H] ≈ −1 dex and solar, with a significant [α/Fe] versus [Fe/H] gradient. While strong contamination from the Galactic Bulge prevents accurate measurement of the (Galactic) north side of the Sgr dSph, the dwarf galaxy can be well approximated by a roughly ovaloid projection of characteristic size 4° × 2°, beyond which the projected stellar density is less than half that of the region surrounding the core. The galaxy's major axis is perpendicular to the Galactic Plane, as in previous studies. We find slight evidence to confirm a metallicity gradient in the Sgr dSph and use isochrones to fit a distance of 24.3 ± 2.3 kpc. We were unable to fully constrain the metallicity distribution of the Sgr dSph due to the Bulge contamination and strong correlation of [α/Fe] with metallicity; however, we find that metal-poor stars ([Fe/H] ≲ −1) make up ≲29 per cent of the Sgr dSph's upper red giant branch population. The Bulge population is best fitted by a younger population with [Fe/H] ≈ 0 and [α/Fe] ≈ 0 or slightly higher. We find no evidence for a split, peanut- or X-shaped Bulge population in this line of sight (l = 5$ $_{.}^{\circ}$$6 ± ∼1°, b = −14$ $_{.}^{\circ}$$1 ± ∼3°).
Fil: McDonald, I.. Jodrell Bank Centre for Astrophysics; Reino Unido
Fil: Zijlstra, A. A.. Jodrell Bank Centre for Astrophysics; Reino Unido
Fil: Sloan, G. C.. Cornell University; Estados Unidos
Fil: Kerins, E. J.. Jodrell Bank Centre for Astrophysics; Reino Unido
Fil: Lagadec, E.. Cornell University; Estados Unidos
Fil: Minniti, Dante. Pontificia Universidad Católica de Chile; Chile
Fil: Santucho, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina
Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina
Fil: Dominguez Romero, Mariano Javier de Leon. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina - Materia
-
stars: late type
stars: post-AGB
stars: evolution
stars: fundamental parameters
Galaxy: bulge
Galaxies: individual
Galaxies: Sgr dSph - 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:11336/26997
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VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic BulgeMcDonald, I.Zijlstra, A. A.Sloan, G. C.Kerins, E. J.Lagadec, E.Minniti, DanteSantucho, María VictoriaGurovich, SebastianDominguez Romero, Mariano Javier de Leonstars: late typestars: post-AGBstars: evolutionstars: fundamental parametersGalaxy: bulgeGalaxies: individualGalaxies: Sgr dSphWe present the deepest near-infrared (ZJKs) photometry yet obtained of the Sagittarius dwarf spheroidal (Sgr dSph), using Visible and Infrared Survey Telescope for Astronomy (VISTA) to survey 11 square degrees centred on its core. We list locations and ZJKs-band magnitudes for over 2.9 million sources in the field. We discuss the isolation of the Sgr dSph from the foreground and Galactic Bulge populations, identify the Sgr dSph's horizontal branch in the near-infrared for the first time and map the density of the galaxy's stars. We present isochrones for the Sgr dSph and Bulge populations. These are consistent with the previously reported properties of the Sgr dSph core: namely that it is dominated by a population between [Fe/H] ≈ −1 dex and solar, with a significant [α/Fe] versus [Fe/H] gradient. While strong contamination from the Galactic Bulge prevents accurate measurement of the (Galactic) north side of the Sgr dSph, the dwarf galaxy can be well approximated by a roughly ovaloid projection of characteristic size 4° × 2°, beyond which the projected stellar density is less than half that of the region surrounding the core. The galaxy's major axis is perpendicular to the Galactic Plane, as in previous studies. We find slight evidence to confirm a metallicity gradient in the Sgr dSph and use isochrones to fit a distance of 24.3 ± 2.3 kpc. We were unable to fully constrain the metallicity distribution of the Sgr dSph due to the Bulge contamination and strong correlation of [α/Fe] with metallicity; however, we find that metal-poor stars ([Fe/H] ≲ −1) make up ≲29 per cent of the Sgr dSph's upper red giant branch population. The Bulge population is best fitted by a younger population with [Fe/H] ≈ 0 and [α/Fe] ≈ 0 or slightly higher. We find no evidence for a split, peanut- or X-shaped Bulge population in this line of sight (l = 5$ $_{.}^{\circ}$$6 ± ∼1°, b = −14$ $_{.}^{\circ}$$1 ± ∼3°).Fil: McDonald, I.. Jodrell Bank Centre for Astrophysics; Reino UnidoFil: Zijlstra, A. A.. Jodrell Bank Centre for Astrophysics; Reino UnidoFil: Sloan, G. C.. Cornell University; Estados UnidosFil: Kerins, E. J.. Jodrell Bank Centre for Astrophysics; Reino UnidoFil: Lagadec, E.. Cornell University; Estados UnidosFil: Minniti, Dante. Pontificia Universidad Católica de Chile; ChileFil: Santucho, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; ArgentinaFil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; ArgentinaFil: Dominguez Romero, Mariano Javier de Leon. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; ArgentinaOxford University Press2013-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/26997McDonald, I.; Zijlstra, A. A.; Sloan, G. C.; Kerins, E. J.; Lagadec, E.; et al.; VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 436; 1; 9-2013; 413-4290035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stt1576info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/436/1/413/973089/VISTA-s-view-of-the-Sagittarius-dwarf-spheroidalinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1308.4323info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:06Zoai:ri.conicet.gov.ar:11336/26997instacron: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 10:04:06.925CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
title |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
spellingShingle |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge McDonald, I. stars: late type stars: post-AGB stars: evolution stars: fundamental parameters Galaxy: bulge Galaxies: individual Galaxies: Sgr dSph |
title_short |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
title_full |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
title_fullStr |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
title_full_unstemmed |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
title_sort |
VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge |
dc.creator.none.fl_str_mv |
McDonald, I. Zijlstra, A. A. Sloan, G. C. Kerins, E. J. Lagadec, E. Minniti, Dante Santucho, María Victoria Gurovich, Sebastian Dominguez Romero, Mariano Javier de Leon |
author |
McDonald, I. |
author_facet |
McDonald, I. Zijlstra, A. A. Sloan, G. C. Kerins, E. J. Lagadec, E. Minniti, Dante Santucho, María Victoria Gurovich, Sebastian Dominguez Romero, Mariano Javier de Leon |
author_role |
author |
author2 |
Zijlstra, A. A. Sloan, G. C. Kerins, E. J. Lagadec, E. Minniti, Dante Santucho, María Victoria Gurovich, Sebastian Dominguez Romero, Mariano Javier de Leon |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
stars: late type stars: post-AGB stars: evolution stars: fundamental parameters Galaxy: bulge Galaxies: individual Galaxies: Sgr dSph |
topic |
stars: late type stars: post-AGB stars: evolution stars: fundamental parameters Galaxy: bulge Galaxies: individual Galaxies: Sgr dSph |
dc.description.none.fl_txt_mv |
We present the deepest near-infrared (ZJKs) photometry yet obtained of the Sagittarius dwarf spheroidal (Sgr dSph), using Visible and Infrared Survey Telescope for Astronomy (VISTA) to survey 11 square degrees centred on its core. We list locations and ZJKs-band magnitudes for over 2.9 million sources in the field. We discuss the isolation of the Sgr dSph from the foreground and Galactic Bulge populations, identify the Sgr dSph's horizontal branch in the near-infrared for the first time and map the density of the galaxy's stars. We present isochrones for the Sgr dSph and Bulge populations. These are consistent with the previously reported properties of the Sgr dSph core: namely that it is dominated by a population between [Fe/H] ≈ −1 dex and solar, with a significant [α/Fe] versus [Fe/H] gradient. While strong contamination from the Galactic Bulge prevents accurate measurement of the (Galactic) north side of the Sgr dSph, the dwarf galaxy can be well approximated by a roughly ovaloid projection of characteristic size 4° × 2°, beyond which the projected stellar density is less than half that of the region surrounding the core. The galaxy's major axis is perpendicular to the Galactic Plane, as in previous studies. We find slight evidence to confirm a metallicity gradient in the Sgr dSph and use isochrones to fit a distance of 24.3 ± 2.3 kpc. We were unable to fully constrain the metallicity distribution of the Sgr dSph due to the Bulge contamination and strong correlation of [α/Fe] with metallicity; however, we find that metal-poor stars ([Fe/H] ≲ −1) make up ≲29 per cent of the Sgr dSph's upper red giant branch population. The Bulge population is best fitted by a younger population with [Fe/H] ≈ 0 and [α/Fe] ≈ 0 or slightly higher. We find no evidence for a split, peanut- or X-shaped Bulge population in this line of sight (l = 5$ $_{.}^{\circ}$$6 ± ∼1°, b = −14$ $_{.}^{\circ}$$1 ± ∼3°). Fil: McDonald, I.. Jodrell Bank Centre for Astrophysics; Reino Unido Fil: Zijlstra, A. A.. Jodrell Bank Centre for Astrophysics; Reino Unido Fil: Sloan, G. C.. Cornell University; Estados Unidos Fil: Kerins, E. J.. Jodrell Bank Centre for Astrophysics; Reino Unido Fil: Lagadec, E.. Cornell University; Estados Unidos Fil: Minniti, Dante. Pontificia Universidad Católica de Chile; Chile Fil: Santucho, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina Fil: Dominguez Romero, Mariano Javier de Leon. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina |
description |
We present the deepest near-infrared (ZJKs) photometry yet obtained of the Sagittarius dwarf spheroidal (Sgr dSph), using Visible and Infrared Survey Telescope for Astronomy (VISTA) to survey 11 square degrees centred on its core. We list locations and ZJKs-band magnitudes for over 2.9 million sources in the field. We discuss the isolation of the Sgr dSph from the foreground and Galactic Bulge populations, identify the Sgr dSph's horizontal branch in the near-infrared for the first time and map the density of the galaxy's stars. We present isochrones for the Sgr dSph and Bulge populations. These are consistent with the previously reported properties of the Sgr dSph core: namely that it is dominated by a population between [Fe/H] ≈ −1 dex and solar, with a significant [α/Fe] versus [Fe/H] gradient. While strong contamination from the Galactic Bulge prevents accurate measurement of the (Galactic) north side of the Sgr dSph, the dwarf galaxy can be well approximated by a roughly ovaloid projection of characteristic size 4° × 2°, beyond which the projected stellar density is less than half that of the region surrounding the core. The galaxy's major axis is perpendicular to the Galactic Plane, as in previous studies. We find slight evidence to confirm a metallicity gradient in the Sgr dSph and use isochrones to fit a distance of 24.3 ± 2.3 kpc. We were unable to fully constrain the metallicity distribution of the Sgr dSph due to the Bulge contamination and strong correlation of [α/Fe] with metallicity; however, we find that metal-poor stars ([Fe/H] ≲ −1) make up ≲29 per cent of the Sgr dSph's upper red giant branch population. The Bulge population is best fitted by a younger population with [Fe/H] ≈ 0 and [α/Fe] ≈ 0 or slightly higher. We find no evidence for a split, peanut- or X-shaped Bulge population in this line of sight (l = 5$ $_{.}^{\circ}$$6 ± ∼1°, b = −14$ $_{.}^{\circ}$$1 ± ∼3°). |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-09 |
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/11336/26997 McDonald, I.; Zijlstra, A. A.; Sloan, G. C.; Kerins, E. J.; Lagadec, E.; et al.; VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 436; 1; 9-2013; 413-429 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/26997 |
identifier_str_mv |
McDonald, I.; Zijlstra, A. A.; Sloan, G. C.; Kerins, E. J.; Lagadec, E.; et al.; VISTA’s view of the Sagittarius dwarf spheroidal galaxy and southern Galactic Bulge; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 436; 1; 9-2013; 413-429 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stt1576 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/436/1/413/973089/VISTA-s-view-of-the-Sagittarius-dwarf-spheroidal info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1308.4323 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
Oxford University Press |
publisher.none.fl_str_mv |
Oxford University Press |
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) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
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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1844613864746909696 |
score |
13.070432 |