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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/129385
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:39:01Zoai: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:34982025-09-29 10:39:02.023CONICET 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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13.070432 |