Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia

Autores
Minniti, Dante; Alonso-Garcia, Javier; Borissova, Jura; Claria Olmedo, Juan Jose; Días, Bruno; Gómez, Matias; Hempel, Maren; Kurtev, Radostin; Palma, Tali; Pullen, Joyce; Saito, Roberto K
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We have extended our previous bulge GC searches following the procedures described by Minniti et al. (2017abc), adding a couple of additional steps to target more distant objects. Considering the high foreground contamination and in order to discard nearby sources, we used the matched VVV-Gaia catalogues of Kammers et al. (2019), with distances DBJ < 3 kpc (Bailer Jones 2018). Also, we rejected sources with proper motions consistent with the mean motion of the Galactic disk for the different fields. We then built red giant density maps and identified the over-densities with sizes typical for GCs. Finally, we checked the optical and near-IR color-magnitude diagrams for all individual objects, selecting the ones with red giant branches tighter than their surrounding fields. While in most targets a clear red clump is present, in a few cases there is also a concentration of RR Lyrae stars and/or a blue horizontal branch can be observed. We found fifty new candidate GCs.
Fil: Minniti, Dante. Universidad Andrés Bello; Chile
Fil: Alonso-Garcia, Javier. Universidad de Antofagasta; Chile
Fil: Borissova, Jura. Universidad de Valparaíso; Chile
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Días, Bruno. Universidad Andrés Bello; Chile
Fil: Gómez, Matias. Universidad Andrés Bello; Chile
Fil: Hempel, Maren. Universidad Andrés Bello; Chile
Fil: Kurtev, Radostin. Universidad de Valparaíso; Chile
Fil: Palma, Tali. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Pullen, Joyce. Universidad Andrés Bello; Chile
Fil: Saito, Roberto K. Universidade Federal de Santa Catarina; Brasil
Materia
GAIA GATALOG
GLOBULAR CLUSTERS
RR LYRAE STARS
VVV SURVEY
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/129385
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/129385
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Fifty star cluster candidates towards the Galactic bulge from VVV and GaiaMinniti, DanteAlonso-Garcia, JavierBorissova, JuraClaria Olmedo, Juan JoseDías, BrunoGómez, MatiasHempel, MarenKurtev, RadostinPalma, TaliPullen, JoyceSaito, Roberto KGAIA GATALOGGLOBULAR CLUSTERSRR LYRAE STARSVVV SURVEYhttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We have extended our previous bulge GC searches following the procedures described by Minniti et al. (2017abc), adding a couple of additional steps to target more distant objects. Considering the high foreground contamination and in order to discard nearby sources, we used the matched VVV-Gaia catalogues of Kammers et al. (2019), with distances DBJ < 3 kpc (Bailer Jones 2018). Also, we rejected sources with proper motions consistent with the mean motion of the Galactic disk for the different fields. We then built red giant density maps and identified the over-densities with sizes typical for GCs. Finally, we checked the optical and near-IR color-magnitude diagrams for all individual objects, selecting the ones with red giant branches tighter than their surrounding fields. While in most targets a clear red clump is present, in a few cases there is also a concentration of RR Lyrae stars and/or a blue horizontal branch can be observed. We found fifty new candidate GCs.Fil: Minniti, Dante. Universidad Andrés Bello; ChileFil: Alonso-Garcia, Javier. Universidad de Antofagasta; ChileFil: Borissova, Jura. Universidad de Valparaíso; ChileFil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Días, Bruno. Universidad Andrés Bello; ChileFil: Gómez, Matias. Universidad Andrés Bello; ChileFil: Hempel, Maren. Universidad Andrés Bello; ChileFil: Kurtev, Radostin. Universidad de Valparaíso; ChileFil: Palma, Tali. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Pullen, Joyce. Universidad Andrés Bello; ChileFil: Saito, Roberto K. Universidade Federal de Santa Catarina; BrasilIOP PUBLISHING LTD2019-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/vnd.openxmlformats-officedocument.wordprocessingml.documentapplication/pdfhttp://hdl.handle.net/11336/129385Minniti, Dante; Alonso-Garcia, Javier; Borissova, Jura; Claria Olmedo, Juan Jose; Días, Bruno; et al.; Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia; IOP PUBLISHING LTD; Research Notes of the AAS; 3; 7; 7-2019; 101-1022515-5172CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2515-5172/ab3391info:eu-repo/semantics/altIdentifier/doi/10.3847/2515-5172/ab3391info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:11:15Zoai:ri.conicet.gov.ar:11336/129385instacron: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:34982025-10-22 12:11:15.552CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
title Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
spellingShingle Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
Minniti, Dante
GAIA GATALOG
GLOBULAR CLUSTERS
RR LYRAE STARS
VVV SURVEY
title_short Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
title_full Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
title_fullStr Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
title_full_unstemmed Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
title_sort Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia
dc.creator.none.fl_str_mv Minniti, Dante
Alonso-Garcia, Javier
Borissova, Jura
Claria Olmedo, Juan Jose
Días, Bruno
Gómez, Matias
Hempel, Maren
Kurtev, Radostin
Palma, Tali
Pullen, Joyce
Saito, Roberto K
author Minniti, Dante
author_facet Minniti, Dante
Alonso-Garcia, Javier
Borissova, Jura
Claria Olmedo, Juan Jose
Días, Bruno
Gómez, Matias
Hempel, Maren
Kurtev, Radostin
Palma, Tali
Pullen, Joyce
Saito, Roberto K
author_role author
author2 Alonso-Garcia, Javier
Borissova, Jura
Claria Olmedo, Juan Jose
Días, Bruno
Gómez, Matias
Hempel, Maren
Kurtev, Radostin
Palma, Tali
Pullen, Joyce
Saito, Roberto K
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GAIA GATALOG
GLOBULAR CLUSTERS
RR LYRAE STARS
VVV SURVEY
topic GAIA GATALOG
GLOBULAR CLUSTERS
RR LYRAE STARS
VVV SURVEY
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We have extended our previous bulge GC searches following the procedures described by Minniti et al. (2017abc), adding a couple of additional steps to target more distant objects. Considering the high foreground contamination and in order to discard nearby sources, we used the matched VVV-Gaia catalogues of Kammers et al. (2019), with distances DBJ < 3 kpc (Bailer Jones 2018). Also, we rejected sources with proper motions consistent with the mean motion of the Galactic disk for the different fields. We then built red giant density maps and identified the over-densities with sizes typical for GCs. Finally, we checked the optical and near-IR color-magnitude diagrams for all individual objects, selecting the ones with red giant branches tighter than their surrounding fields. While in most targets a clear red clump is present, in a few cases there is also a concentration of RR Lyrae stars and/or a blue horizontal branch can be observed. We found fifty new candidate GCs.
Fil: Minniti, Dante. Universidad Andrés Bello; Chile
Fil: Alonso-Garcia, Javier. Universidad de Antofagasta; Chile
Fil: Borissova, Jura. Universidad de Valparaíso; Chile
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Días, Bruno. Universidad Andrés Bello; Chile
Fil: Gómez, Matias. Universidad Andrés Bello; Chile
Fil: Hempel, Maren. Universidad Andrés Bello; Chile
Fil: Kurtev, Radostin. Universidad de Valparaíso; Chile
Fil: Palma, Tali. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Pullen, Joyce. Universidad Andrés Bello; Chile
Fil: Saito, Roberto K. Universidade Federal de Santa Catarina; Brasil
description We have extended our previous bulge GC searches following the procedures described by Minniti et al. (2017abc), adding a couple of additional steps to target more distant objects. Considering the high foreground contamination and in order to discard nearby sources, we used the matched VVV-Gaia catalogues of Kammers et al. (2019), with distances DBJ < 3 kpc (Bailer Jones 2018). Also, we rejected sources with proper motions consistent with the mean motion of the Galactic disk for the different fields. We then built red giant density maps and identified the over-densities with sizes typical for GCs. Finally, we checked the optical and near-IR color-magnitude diagrams for all individual objects, selecting the ones with red giant branches tighter than their surrounding fields. While in most targets a clear red clump is present, in a few cases there is also a concentration of RR Lyrae stars and/or a blue horizontal branch can be observed. We found fifty new candidate GCs.
publishDate 2019
dc.date.none.fl_str_mv 2019-07
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/11336/129385
Minniti, Dante; Alonso-Garcia, Javier; Borissova, Jura; Claria Olmedo, Juan Jose; Días, Bruno; et al.; Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia; IOP PUBLISHING LTD; Research Notes of the AAS; 3; 7; 7-2019; 101-102
2515-5172
CONICET Digital
CONICET
url http://hdl.handle.net/11336/129385
identifier_str_mv Minniti, Dante; Alonso-Garcia, Javier; Borissova, Jura; Claria Olmedo, Juan Jose; Días, Bruno; et al.; Fifty star cluster candidates towards the Galactic bulge from VVV and Gaia; IOP PUBLISHING LTD; Research Notes of the AAS; 3; 7; 7-2019; 101-102
2515-5172
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/2515-5172/ab3391
info:eu-repo/semantics/altIdentifier/doi/10.3847/2515-5172/ab3391
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/vnd.openxmlformats-officedocument.wordprocessingml.document
application/pdf
dc.publisher.none.fl_str_mv IOP PUBLISHING LTD
publisher.none.fl_str_mv IOP PUBLISHING LTD
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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score 12.982451

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