Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates

Autores
Bedin, L.R.; Piotto, G.; Baume, Gustavo Luis; Momany, Y.; Carraro, Giovanni; Anderson, J.; Messineo, M.; Ortolani, S.
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this work we present the detection of 33 star clusters and 51 candidates in one field of the near by galaxy M 33. This study is based on WFC/ACS images available from the HST archive. Thanks to the high resolving power, we were able to confirm that two candidates previously indicated by Christian & Schommer (1982, ApJS, 49, 405) are indeed star clusters. We list the main properties for the star clusters (and candidates), along with some peculiar objects, such as background galaxies and possible HII regions. © ESO 2005.
Fil: Bedin, L.R.. European Southern Observatory;
Fil: Piotto, G.. Università di Padova; Italia
Fil: Baume, Gustavo Luis. Università di Padova; Italia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Momany, Y.. Università di Padova; Italia
Fil: Carraro, Giovanni. Università di Padova; Italia. Universidad de Chile; Chile
Fil: Anderson, J.. Rice University; Estados Unidos
Fil: Messineo, M.. European Southern Observatory;
Fil: Ortolani, S.. Università di Padova; Italia
Materia
Star clusters
M 33 (galxia)
Galaxies
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:11336/38890

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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidatesBedin, L.R.Piotto, G.Baume, Gustavo LuisMomany, Y.Carraro, GiovanniAnderson, J.Messineo, M.Ortolani, S.Star clustersM 33 (galxia)Galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work we present the detection of 33 star clusters and 51 candidates in one field of the near by galaxy M 33. This study is based on WFC/ACS images available from the HST archive. Thanks to the high resolving power, we were able to confirm that two candidates previously indicated by Christian & Schommer (1982, ApJS, 49, 405) are indeed star clusters. We list the main properties for the star clusters (and candidates), along with some peculiar objects, such as background galaxies and possible HII regions. © ESO 2005.Fil: Bedin, L.R.. European Southern Observatory;Fil: Piotto, G.. Università di Padova; ItaliaFil: Baume, Gustavo Luis. Università di Padova; Italia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Momany, Y.. Università di Padova; ItaliaFil: Carraro, Giovanni. Università di Padova; Italia. Universidad de Chile; ChileFil: Anderson, J.. Rice University; Estados UnidosFil: Messineo, M.. European Southern Observatory;Fil: Ortolani, S.. Università di Padova; ItaliaEDP Sciences2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/38890Bedin, L.R.; Piotto, G.; Baume, Gustavo Luis; Momany, Y.; Carraro, Giovanni; et al.; Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates; EDP Sciences; Astronomy and Astrophysics; 444; 3; 12-2005; 831-8360004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20053700info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2005/48/aa3700-05/aa3700-05.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-06-10T09:59:23Zoai:ri.conicet.gov.ar:11336/38890instacron: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:34982026-06-10 09:59:24.125CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
title Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
spellingShingle Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
Bedin, L.R.
Star clusters
M 33 (galxia)
Galaxies
title_short Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
title_full Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
title_fullStr Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
title_full_unstemmed Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
title_sort Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates
dc.creator.none.fl_str_mv Bedin, L.R.
Piotto, G.
Baume, Gustavo Luis
Momany, Y.
Carraro, Giovanni
Anderson, J.
Messineo, M.
Ortolani, S.
author Bedin, L.R.
author_facet Bedin, L.R.
Piotto, G.
Baume, Gustavo Luis
Momany, Y.
Carraro, Giovanni
Anderson, J.
Messineo, M.
Ortolani, S.
author_role author
author2 Piotto, G.
Baume, Gustavo Luis
Momany, Y.
Carraro, Giovanni
Anderson, J.
Messineo, M.
Ortolani, S.
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Star clusters
M 33 (galxia)
Galaxies
topic Star clusters
M 33 (galxia)
Galaxies
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this work we present the detection of 33 star clusters and 51 candidates in one field of the near by galaxy M 33. This study is based on WFC/ACS images available from the HST archive. Thanks to the high resolving power, we were able to confirm that two candidates previously indicated by Christian & Schommer (1982, ApJS, 49, 405) are indeed star clusters. We list the main properties for the star clusters (and candidates), along with some peculiar objects, such as background galaxies and possible HII regions. © ESO 2005.
Fil: Bedin, L.R.. European Southern Observatory;
Fil: Piotto, G.. Università di Padova; Italia
Fil: Baume, Gustavo Luis. Università di Padova; Italia. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Momany, Y.. Università di Padova; Italia
Fil: Carraro, Giovanni. Università di Padova; Italia. Universidad de Chile; Chile
Fil: Anderson, J.. Rice University; Estados Unidos
Fil: Messineo, M.. European Southern Observatory;
Fil: Ortolani, S.. Università di Padova; Italia
description In this work we present the detection of 33 star clusters and 51 candidates in one field of the near by galaxy M 33. This study is based on WFC/ACS images available from the HST archive. Thanks to the high resolving power, we were able to confirm that two candidates previously indicated by Christian & Schommer (1982, ApJS, 49, 405) are indeed star clusters. We list the main properties for the star clusters (and candidates), along with some peculiar objects, such as background galaxies and possible HII regions. © ESO 2005.
publishDate 2005
dc.date.none.fl_str_mv 2005-12
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/11336/38890
Bedin, L.R.; Piotto, G.; Baume, Gustavo Luis; Momany, Y.; Carraro, Giovanni; et al.; Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates; EDP Sciences; Astronomy and Astrophysics; 444; 3; 12-2005; 831-836
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/38890
identifier_str_mv Bedin, L.R.; Piotto, G.; Baume, Gustavo Luis; Momany, Y.; Carraro, Giovanni; et al.; Star cluster detection with WFC/ACS in M 33, 33 new clusters and 51 candidates; EDP Sciences; Astronomy and Astrophysics; 444; 3; 12-2005; 831-836
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20053700
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2005/48/aa3700-05/aa3700-05.html
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 EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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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