A deep and wide-field view at the IC 2944/2948 complex in Centaurus
- Autores
- Baume, Gustavo Luis; Rodriguez, Maria Jimena; Corti, Mariela Alejandra; Carraro, Giovanni; Panei, Jorge Alejandro
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We employed the ESO MPI wide-field camera and obtained deep images in the VIC passbands in the region of the IC 2944/2948 complex (l∼294.º 8; b∼−1.6º), and complemented them with literature and archival data. We used this material to derive the photometric, spectroscopic and kinematic properties of the brightest (V < 16) stars in the region. The VI deep photometry on the other end, helped us to unravel the lower main sequence of a few, possibly physical, star groups in the area. Our analysis confirmed previous suggestions that the extinction toward this line of sight follows the normal law (RV=3.1). We could recognize B-type stars spread in distance from a few hundred pc to at least 2 kpc. We found two young groups (age∼3 Myr) located respectively at about 2.3 and 3.2 kpc from the Sun. They are characterized by a significant variable extinction (E(B−V) ranging from 0.28 to 0.45 mag), and host a significant pre-main sequence population. We computed the initial mass functions for these groups and obtained slopes Gamma from -0.94 to -1.02 (e_Gamma=0.3), in a scale where the classical Salpeter law is -1.35. We estimated the total mass of both main stellar groups in ∼1100 and ∼500 M_sun, respectively. Our kinematic analysis indicated that both groups of stars deviate from the standard rotation curve of the Milky Way, in line with literature results for this specific Galactic direction. Finally, along the same line of sight we identified a third group of early-type stars located at ∼8 kpc from the Sun. This group might be located in the far side of the Sagittarius-Carina spiral arm.
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: Rodriguez, Maria Jimena. 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: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Carraro, Giovanni. European Southern Observatory; Chile
Fil: Panei, Jorge Alejandro. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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 - Materia
-
Open clusters and associations
IC 2944 (astronomía)
Galactic Structure
Early type stars
IC 2948 (astronomía)
Centaurus - 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:11336/23683
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A deep and wide-field view at the IC 2944/2948 complex in CentaurusBaume, Gustavo LuisRodriguez, Maria JimenaCorti, Mariela AlejandraCarraro, GiovanniPanei, Jorge AlejandroOpen clusters and associationsIC 2944 (astronomía)Galactic StructureEarly type starsIC 2948 (astronomía)Centaurushttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We employed the ESO MPI wide-field camera and obtained deep images in the VIC passbands in the region of the IC 2944/2948 complex (l∼294.º 8; b∼−1.6º), and complemented them with literature and archival data. We used this material to derive the photometric, spectroscopic and kinematic properties of the brightest (V < 16) stars in the region. The VI deep photometry on the other end, helped us to unravel the lower main sequence of a few, possibly physical, star groups in the area. Our analysis confirmed previous suggestions that the extinction toward this line of sight follows the normal law (RV=3.1). We could recognize B-type stars spread in distance from a few hundred pc to at least 2 kpc. We found two young groups (age∼3 Myr) located respectively at about 2.3 and 3.2 kpc from the Sun. They are characterized by a significant variable extinction (E(B−V) ranging from 0.28 to 0.45 mag), and host a significant pre-main sequence population. We computed the initial mass functions for these groups and obtained slopes Gamma from -0.94 to -1.02 (e_Gamma=0.3), in a scale where the classical Salpeter law is -1.35. We estimated the total mass of both main stellar groups in ∼1100 and ∼500 M_sun, respectively. Our kinematic analysis indicated that both groups of stars deviate from the standard rotation curve of the Milky Way, in line with literature results for this specific Galactic direction. Finally, along the same line of sight we identified a third group of early-type stars located at ∼8 kpc from the Sun. This group might be located in the far side of the Sagittarius-Carina spiral arm.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; ArgentinaFil: Rodriguez, Maria Jimena. 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: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Carraro, Giovanni. European Southern Observatory; ChileFil: Panei, Jorge Alejandro. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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; ArgentinaOxford University Press2014-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/23683Baume, Gustavo Luis; Rodriguez, Maria Jimena; Corti, Mariela Alejandra; Carraro, Giovanni; Panei, Jorge Alejandro; A deep and wide-field view at the IC 2944/2948 complex in Centaurus; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 443; 9-2014; 411-4220035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stu1108info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stu1108info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:49:31Zoai:ri.conicet.gov.ar:11336/23683instacron: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 09:49:31.67CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
title |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
spellingShingle |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus Baume, Gustavo Luis Open clusters and associations IC 2944 (astronomía) Galactic Structure Early type stars IC 2948 (astronomía) Centaurus |
title_short |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
title_full |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
title_fullStr |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
title_full_unstemmed |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
title_sort |
A deep and wide-field view at the IC 2944/2948 complex in Centaurus |
dc.creator.none.fl_str_mv |
Baume, Gustavo Luis Rodriguez, Maria Jimena Corti, Mariela Alejandra Carraro, Giovanni Panei, Jorge Alejandro |
author |
Baume, Gustavo Luis |
author_facet |
Baume, Gustavo Luis Rodriguez, Maria Jimena Corti, Mariela Alejandra Carraro, Giovanni Panei, Jorge Alejandro |
author_role |
author |
author2 |
Rodriguez, Maria Jimena Corti, Mariela Alejandra Carraro, Giovanni Panei, Jorge Alejandro |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Open clusters and associations IC 2944 (astronomía) Galactic Structure Early type stars IC 2948 (astronomía) Centaurus |
topic |
Open clusters and associations IC 2944 (astronomía) Galactic Structure Early type stars IC 2948 (astronomía) Centaurus |
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 employed the ESO MPI wide-field camera and obtained deep images in the VIC passbands in the region of the IC 2944/2948 complex (l∼294.º 8; b∼−1.6º), and complemented them with literature and archival data. We used this material to derive the photometric, spectroscopic and kinematic properties of the brightest (V < 16) stars in the region. The VI deep photometry on the other end, helped us to unravel the lower main sequence of a few, possibly physical, star groups in the area. Our analysis confirmed previous suggestions that the extinction toward this line of sight follows the normal law (RV=3.1). We could recognize B-type stars spread in distance from a few hundred pc to at least 2 kpc. We found two young groups (age∼3 Myr) located respectively at about 2.3 and 3.2 kpc from the Sun. They are characterized by a significant variable extinction (E(B−V) ranging from 0.28 to 0.45 mag), and host a significant pre-main sequence population. We computed the initial mass functions for these groups and obtained slopes Gamma from -0.94 to -1.02 (e_Gamma=0.3), in a scale where the classical Salpeter law is -1.35. We estimated the total mass of both main stellar groups in ∼1100 and ∼500 M_sun, respectively. Our kinematic analysis indicated that both groups of stars deviate from the standard rotation curve of the Milky Way, in line with literature results for this specific Galactic direction. Finally, along the same line of sight we identified a third group of early-type stars located at ∼8 kpc from the Sun. This group might be located in the far side of the Sagittarius-Carina spiral arm. 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: Rodriguez, Maria Jimena. 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: Corti, Mariela Alejandra. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Carraro, Giovanni. European Southern Observatory; Chile Fil: Panei, Jorge Alejandro. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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 |
description |
We employed the ESO MPI wide-field camera and obtained deep images in the VIC passbands in the region of the IC 2944/2948 complex (l∼294.º 8; b∼−1.6º), and complemented them with literature and archival data. We used this material to derive the photometric, spectroscopic and kinematic properties of the brightest (V < 16) stars in the region. The VI deep photometry on the other end, helped us to unravel the lower main sequence of a few, possibly physical, star groups in the area. Our analysis confirmed previous suggestions that the extinction toward this line of sight follows the normal law (RV=3.1). We could recognize B-type stars spread in distance from a few hundred pc to at least 2 kpc. We found two young groups (age∼3 Myr) located respectively at about 2.3 and 3.2 kpc from the Sun. They are characterized by a significant variable extinction (E(B−V) ranging from 0.28 to 0.45 mag), and host a significant pre-main sequence population. We computed the initial mass functions for these groups and obtained slopes Gamma from -0.94 to -1.02 (e_Gamma=0.3), in a scale where the classical Salpeter law is -1.35. We estimated the total mass of both main stellar groups in ∼1100 and ∼500 M_sun, respectively. Our kinematic analysis indicated that both groups of stars deviate from the standard rotation curve of the Milky Way, in line with literature results for this specific Galactic direction. Finally, along the same line of sight we identified a third group of early-type stars located at ∼8 kpc from the Sun. This group might be located in the far side of the Sagittarius-Carina spiral arm. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-09 |
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/11336/23683 Baume, Gustavo Luis; Rodriguez, Maria Jimena; Corti, Mariela Alejandra; Carraro, Giovanni; Panei, Jorge Alejandro; A deep and wide-field view at the IC 2944/2948 complex in Centaurus; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 443; 9-2014; 411-422 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/23683 |
identifier_str_mv |
Baume, Gustavo Luis; Rodriguez, Maria Jimena; Corti, Mariela Alejandra; Carraro, Giovanni; Panei, Jorge Alejandro; A deep and wide-field view at the IC 2944/2948 complex in Centaurus; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 443; 9-2014; 411-422 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stu1108 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stu1108 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
Oxford University Press |
publisher.none.fl_str_mv |
Oxford University Press |
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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1844613532939714560 |
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13.070432 |