The line-of-sight depth of popuous clusters in the Small Magellanic Cloud
- Autores
- Crowl, Hugh H.; Sarajedini, Ata; Piatti, Andres Eduardo; Geisler, Doug; Bica, Eduardo; Claria Olmedo, Juan Jose; Santos Jr., João F. C.
- Año de publicación
- 2001
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present an analysis of age, metal abundance and positional data on populous clusters in the Small Magellanic Cloud (SMC) with the ultimate aim of determining the line-of-sight (LOS) depth of the SMC by using these clusters as proxies. Our data set contains 12 objects and is limited to clusters with the highest-quality data for which the ages and abundances are best known and can be placed on an internally consistent scale. We have analyzed the variation of the clusters´ properties with position on the sky and with LOS depth. Based on this analysis, we draw the following conclusions: (1) The observational data indicate that the eastern side of the SMC (facing the large Magellanic Cloud) contains younger and more metal-rich clusters as compared with the western side. This is not a strong correlation because our data set of clusters is necessarily limited, but is suggestive and warrants further studyl. (2) Depending on how the reddening is computed to our clusters, we find a mean distance modulus that ranges from (m-M)o = 18.71 +/- 0.06 to 18.82 +/- 0.05. (3) The intrinsic +/- 1 sigma LOS depth of the SMC populous clusters in our study is between 6 and approximately 12 kpc, depending primarily on whether we adopt the Burstein & Heiles reddenings or those from Schlegel et al. (4) Viewing the SMC as a triaxial galaxy with declination, right ascension and LOS depth as the three axes, we find axial ratios of approximately 1:2:4. Taken together, these conclusions largely agree with those of previous investigator sand underscore the utility of populous star clusters as probes of the structure of the SMC.
Fil: Crowl, Hugh H.. Wesleyan University; Estados Unidos
Fil: Sarajedini, Ata. Wesleyan University; Estados Unidos
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Geisler, Doug. Universidad de Concepción; Chile
Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Fil: Santos Jr., João F. C.. Universidade Federal do Minas Gerais; Brasil - Materia
-
Small Magellanic Cloud
Star cluster
Photometry - 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:11336/22468
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The line-of-sight depth of popuous clusters in the Small Magellanic CloudCrowl, Hugh H.Sarajedini, AtaPiatti, Andres EduardoGeisler, DougBica, EduardoClaria Olmedo, Juan JoseSantos Jr., João F. C.Small Magellanic CloudStar clusterPhotometryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an analysis of age, metal abundance and positional data on populous clusters in the Small Magellanic Cloud (SMC) with the ultimate aim of determining the line-of-sight (LOS) depth of the SMC by using these clusters as proxies. Our data set contains 12 objects and is limited to clusters with the highest-quality data for which the ages and abundances are best known and can be placed on an internally consistent scale. We have analyzed the variation of the clusters´ properties with position on the sky and with LOS depth. Based on this analysis, we draw the following conclusions: (1) The observational data indicate that the eastern side of the SMC (facing the large Magellanic Cloud) contains younger and more metal-rich clusters as compared with the western side. This is not a strong correlation because our data set of clusters is necessarily limited, but is suggestive and warrants further studyl. (2) Depending on how the reddening is computed to our clusters, we find a mean distance modulus that ranges from (m-M)o = 18.71 +/- 0.06 to 18.82 +/- 0.05. (3) The intrinsic +/- 1 sigma LOS depth of the SMC populous clusters in our study is between 6 and approximately 12 kpc, depending primarily on whether we adopt the Burstein & Heiles reddenings or those from Schlegel et al. (4) Viewing the SMC as a triaxial galaxy with declination, right ascension and LOS depth as the three axes, we find axial ratios of approximately 1:2:4. Taken together, these conclusions largely agree with those of previous investigator sand underscore the utility of populous star clusters as probes of the structure of the SMC.Fil: Crowl, Hugh H.. Wesleyan University; Estados UnidosFil: Sarajedini, Ata. Wesleyan University; Estados UnidosFil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Geisler, Doug. Universidad de Concepción; ChileFil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; BrasilFil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaFil: Santos Jr., João F. C.. Universidade Federal do Minas Gerais; BrasilIOP Publishing2001-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/22468Crowl, Hugh H.; Sarajedini, Ata; Piatti, Andres Eduardo; Geisler, Doug; Bica, Eduardo; et al.; The line-of-sight depth of popuous clusters in the Small Magellanic Cloud; IOP Publishing; Astronomical Journal; 122; 1; 7-2001; 220-2310004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/321128info:eu-repo/semantics/altIdentifier/doi/10.1086/321128info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0104227info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:45:58Zoai:ri.conicet.gov.ar:11336/22468instacron: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 09:45:59.143CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
title |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
spellingShingle |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud Crowl, Hugh H. Small Magellanic Cloud Star cluster Photometry |
title_short |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
title_full |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
title_fullStr |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
title_full_unstemmed |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
title_sort |
The line-of-sight depth of popuous clusters in the Small Magellanic Cloud |
dc.creator.none.fl_str_mv |
Crowl, Hugh H. Sarajedini, Ata Piatti, Andres Eduardo Geisler, Doug Bica, Eduardo Claria Olmedo, Juan Jose Santos Jr., João F. C. |
author |
Crowl, Hugh H. |
author_facet |
Crowl, Hugh H. Sarajedini, Ata Piatti, Andres Eduardo Geisler, Doug Bica, Eduardo Claria Olmedo, Juan Jose Santos Jr., João F. C. |
author_role |
author |
author2 |
Sarajedini, Ata Piatti, Andres Eduardo Geisler, Doug Bica, Eduardo Claria Olmedo, Juan Jose Santos Jr., João F. C. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
Small Magellanic Cloud Star cluster Photometry |
topic |
Small Magellanic Cloud Star cluster Photometry |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present an analysis of age, metal abundance and positional data on populous clusters in the Small Magellanic Cloud (SMC) with the ultimate aim of determining the line-of-sight (LOS) depth of the SMC by using these clusters as proxies. Our data set contains 12 objects and is limited to clusters with the highest-quality data for which the ages and abundances are best known and can be placed on an internally consistent scale. We have analyzed the variation of the clusters´ properties with position on the sky and with LOS depth. Based on this analysis, we draw the following conclusions: (1) The observational data indicate that the eastern side of the SMC (facing the large Magellanic Cloud) contains younger and more metal-rich clusters as compared with the western side. This is not a strong correlation because our data set of clusters is necessarily limited, but is suggestive and warrants further studyl. (2) Depending on how the reddening is computed to our clusters, we find a mean distance modulus that ranges from (m-M)o = 18.71 +/- 0.06 to 18.82 +/- 0.05. (3) The intrinsic +/- 1 sigma LOS depth of the SMC populous clusters in our study is between 6 and approximately 12 kpc, depending primarily on whether we adopt the Burstein & Heiles reddenings or those from Schlegel et al. (4) Viewing the SMC as a triaxial galaxy with declination, right ascension and LOS depth as the three axes, we find axial ratios of approximately 1:2:4. Taken together, these conclusions largely agree with those of previous investigator sand underscore the utility of populous star clusters as probes of the structure of the SMC. Fil: Crowl, Hugh H.. Wesleyan University; Estados Unidos Fil: Sarajedini, Ata. Wesleyan University; Estados Unidos Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Geisler, Doug. Universidad de Concepción; Chile Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina Fil: Santos Jr., João F. C.. Universidade Federal do Minas Gerais; Brasil |
description |
We present an analysis of age, metal abundance and positional data on populous clusters in the Small Magellanic Cloud (SMC) with the ultimate aim of determining the line-of-sight (LOS) depth of the SMC by using these clusters as proxies. Our data set contains 12 objects and is limited to clusters with the highest-quality data for which the ages and abundances are best known and can be placed on an internally consistent scale. We have analyzed the variation of the clusters´ properties with position on the sky and with LOS depth. Based on this analysis, we draw the following conclusions: (1) The observational data indicate that the eastern side of the SMC (facing the large Magellanic Cloud) contains younger and more metal-rich clusters as compared with the western side. This is not a strong correlation because our data set of clusters is necessarily limited, but is suggestive and warrants further studyl. (2) Depending on how the reddening is computed to our clusters, we find a mean distance modulus that ranges from (m-M)o = 18.71 +/- 0.06 to 18.82 +/- 0.05. (3) The intrinsic +/- 1 sigma LOS depth of the SMC populous clusters in our study is between 6 and approximately 12 kpc, depending primarily on whether we adopt the Burstein & Heiles reddenings or those from Schlegel et al. (4) Viewing the SMC as a triaxial galaxy with declination, right ascension and LOS depth as the three axes, we find axial ratios of approximately 1:2:4. Taken together, these conclusions largely agree with those of previous investigator sand underscore the utility of populous star clusters as probes of the structure of the SMC. |
publishDate |
2001 |
dc.date.none.fl_str_mv |
2001-07 |
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/11336/22468 Crowl, Hugh H.; Sarajedini, Ata; Piatti, Andres Eduardo; Geisler, Doug; Bica, Eduardo; et al.; The line-of-sight depth of popuous clusters in the Small Magellanic Cloud; IOP Publishing; Astronomical Journal; 122; 1; 7-2001; 220-231 0004-6256 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/22468 |
identifier_str_mv |
Crowl, Hugh H.; Sarajedini, Ata; Piatti, Andres Eduardo; Geisler, Doug; Bica, Eduardo; et al.; The line-of-sight depth of popuous clusters in the Small Magellanic Cloud; IOP Publishing; Astronomical Journal; 122; 1; 7-2001; 220-231 0004-6256 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/321128 info:eu-repo/semantics/altIdentifier/doi/10.1086/321128 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0104227 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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1844613436749643776 |
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13.070432 |