On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data
- Autores
- Carraro, Giovanni; Baume, Gustavo Luis; Seleznev, Anton F.; Costa, Edgardo
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Our knowledge of stellar evolution and of the structure and chemical evolution of the Galactic disk largely builds on the study of open star clusters. Because of their crucial role in these relevant topics, large homogeneous catalogues of open cluster parameters are highly desirable. Although efforts have been made to develop automatic tools to analyse large numbers of clusters, the results obtained so far vary from study to study, and sometimes are very contradictory when compared to dedicated studies of individual clusters. In this work we highlight the common causes of these discrepancies for some open clusters, and show that at present dedicated studies yield a much better assessment of the nature of star clusters, even in the absence of ideal data-sets. We make use of deep, wide-field, multi-colour photometry to discuss the nature of six strategically selected open star clusters: Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10 and Pismis 14. We have precisely derived their basic parameters by means of a combination of star counts and photometric diagrams. Trumpler 22 and Lynga 6 are included in our study because they are widely known, and thus provided a check of our data and methodology. The remaining four clusters are very poorly known, and their available parameters have been obtained using automatic tools only. Our results are in some cases in severe disagreement with those from automatic surveys.
Fil: Carraro, Giovanni. Università di Padova; Italia
Fil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Seleznev, Anton F.. Ural Federal University; Rusia
Fil: Costa, Edgardo. Universidad de Chile; Chile - Materia
-
Open Clusters: General
Open Clusters: Individual (Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10, Pismis 14) - 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:11336/39892
Ver los metadatos del registro completo
id |
CONICETDig_a9d57d6eb35ba7799aceba122f2f9cb0 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/39892 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited dataCarraro, GiovanniBaume, Gustavo LuisSeleznev, Anton F.Costa, EdgardoOpen Clusters: GeneralOpen Clusters: Individual (Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10, Pismis 14)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Our knowledge of stellar evolution and of the structure and chemical evolution of the Galactic disk largely builds on the study of open star clusters. Because of their crucial role in these relevant topics, large homogeneous catalogues of open cluster parameters are highly desirable. Although efforts have been made to develop automatic tools to analyse large numbers of clusters, the results obtained so far vary from study to study, and sometimes are very contradictory when compared to dedicated studies of individual clusters. In this work we highlight the common causes of these discrepancies for some open clusters, and show that at present dedicated studies yield a much better assessment of the nature of star clusters, even in the absence of ideal data-sets. We make use of deep, wide-field, multi-colour photometry to discuss the nature of six strategically selected open star clusters: Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10 and Pismis 14. We have precisely derived their basic parameters by means of a combination of star counts and photometric diagrams. Trumpler 22 and Lynga 6 are included in our study because they are widely known, and thus provided a check of our data and methodology. The remaining four clusters are very poorly known, and their available parameters have been obtained using automatic tools only. Our results are in some cases in severe disagreement with those from automatic surveys.Fil: Carraro, Giovanni. Università di Padova; ItaliaFil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Seleznev, Anton F.. Ural Federal University; RusiaFil: Costa, Edgardo. Universidad de Chile; ChileSpringer2017-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/39892Carraro, Giovanni; Baume, Gustavo Luis; Seleznev, Anton F.; Costa, Edgardo; On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data; Springer; Astrophysics And Space Science; 362; 7; 7-20170004-640XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-017-3110-3info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs10509-017-3110-3info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:30Zoai:ri.conicet.gov.ar:11336/39892instacron: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 09:36:31.087CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
title |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
spellingShingle |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data Carraro, Giovanni Open Clusters: General Open Clusters: Individual (Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10, Pismis 14) |
title_short |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
title_full |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
title_fullStr |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
title_full_unstemmed |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
title_sort |
On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data |
dc.creator.none.fl_str_mv |
Carraro, Giovanni Baume, Gustavo Luis Seleznev, Anton F. Costa, Edgardo |
author |
Carraro, Giovanni |
author_facet |
Carraro, Giovanni Baume, Gustavo Luis Seleznev, Anton F. Costa, Edgardo |
author_role |
author |
author2 |
Baume, Gustavo Luis Seleznev, Anton F. Costa, Edgardo |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Open Clusters: General Open Clusters: Individual (Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10, Pismis 14) |
topic |
Open Clusters: General Open Clusters: Individual (Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10, Pismis 14) |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Our knowledge of stellar evolution and of the structure and chemical evolution of the Galactic disk largely builds on the study of open star clusters. Because of their crucial role in these relevant topics, large homogeneous catalogues of open cluster parameters are highly desirable. Although efforts have been made to develop automatic tools to analyse large numbers of clusters, the results obtained so far vary from study to study, and sometimes are very contradictory when compared to dedicated studies of individual clusters. In this work we highlight the common causes of these discrepancies for some open clusters, and show that at present dedicated studies yield a much better assessment of the nature of star clusters, even in the absence of ideal data-sets. We make use of deep, wide-field, multi-colour photometry to discuss the nature of six strategically selected open star clusters: Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10 and Pismis 14. We have precisely derived their basic parameters by means of a combination of star counts and photometric diagrams. Trumpler 22 and Lynga 6 are included in our study because they are widely known, and thus provided a check of our data and methodology. The remaining four clusters are very poorly known, and their available parameters have been obtained using automatic tools only. Our results are in some cases in severe disagreement with those from automatic surveys. Fil: Carraro, Giovanni. Università di Padova; Italia Fil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Seleznev, Anton F.. Ural Federal University; Rusia Fil: Costa, Edgardo. Universidad de Chile; Chile |
description |
Our knowledge of stellar evolution and of the structure and chemical evolution of the Galactic disk largely builds on the study of open star clusters. Because of their crucial role in these relevant topics, large homogeneous catalogues of open cluster parameters are highly desirable. Although efforts have been made to develop automatic tools to analyse large numbers of clusters, the results obtained so far vary from study to study, and sometimes are very contradictory when compared to dedicated studies of individual clusters. In this work we highlight the common causes of these discrepancies for some open clusters, and show that at present dedicated studies yield a much better assessment of the nature of star clusters, even in the absence of ideal data-sets. We make use of deep, wide-field, multi-colour photometry to discuss the nature of six strategically selected open star clusters: Trumpler 22, Lynga 6, Hogg 19, Hogg 21, Pismis 10 and Pismis 14. We have precisely derived their basic parameters by means of a combination of star counts and photometric diagrams. Trumpler 22 and Lynga 6 are included in our study because they are widely known, and thus provided a check of our data and methodology. The remaining four clusters are very poorly known, and their available parameters have been obtained using automatic tools only. Our results are in some cases in severe disagreement with those from automatic surveys. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-07 |
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/11336/39892 Carraro, Giovanni; Baume, Gustavo Luis; Seleznev, Anton F.; Costa, Edgardo; On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data; Springer; Astrophysics And Space Science; 362; 7; 7-2017 0004-640X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/39892 |
identifier_str_mv |
Carraro, Giovanni; Baume, Gustavo Luis; Seleznev, Anton F.; Costa, Edgardo; On the assessment of the nature of open star clusters and the determination of their basic parameters with limited data; Springer; Astrophysics And Space Science; 362; 7; 7-2017 0004-640X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-017-3110-3 info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs10509-017-3110-3 |
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 |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
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 |
_version_ |
1844613145544359936 |
score |
13.070432 |