Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA

Autores
Perren, Gabriel Ignacio; Giorgi, Edgard Ervar Salvador; Pera, María Sol; Navone, Hugo Daniel; Cruzado, Alicia; Vázquez, Rubén Ángel
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The fine structure of the open cluster NGC 2516 is investigated. This is an extended and relatively young open cluster subtending over two degrees in the sky, situated at just a few hundred PARSECs (< 400 pc) from the Sun. We collected Gaia DR2 data (G magnitude down to G=19, BP-RP color index, proper motions, and parallaxes) for more than 400 000 stars in a region of 6 degrees on a side, and applied our membership algorithm pyUPMASK. GAIA data for the most probable members was cross-matched with available UBVI data. Finally, we run our ASteCA code to obtain the fundamental cluster parameters.
Investigamos la estructura fina del cúmulo abierto NGC 2516. Este es un cúmulo abierto extendido y relativamente joven que subtiende más de dos grados en el cielo, situado a unos pocos cientos de PARSECs (< 400 pc) del Sol. Recopilamos datos de Gaia DR2 (magnitud G hasta G=19, índice de color BP-RP, movimientos propios y paralaje) para más de 400 000 estrellas en una región de 6 grados de lado, y aplicamos nuestro algoritmo de membresía pyUPMASK. Los datos de GAIA para los miembros más probables se correlacionaron con fotometría UBVI. Finalmente, usamos nuestro código ASteCA para obtener los parámetros fundamentales del cúmulo.
Asociación Argentina de Astronomía
Materia
Ciencias Astronómicas
galaxies: star clusters: general
open clusters and associations: general
techniques: photometric
methods: statistical
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/168382
Acceder
id SEDICI_c3601e8e4f908989a87f2d660bf2584b
oai_identifier_str oai:sedici.unlp.edu.ar:10915/168382
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCAPerren, Gabriel IgnacioGiorgi, Edgard Ervar SalvadorPera, María SolNavone, Hugo DanielCruzado, AliciaVázquez, Rubén ÁngelCiencias Astronómicasgalaxies: star clusters: generalopen clusters and associations: generaltechniques: photometricmethods: statisticalThe fine structure of the open cluster NGC 2516 is investigated. This is an extended and relatively young open cluster subtending over two degrees in the sky, situated at just a few hundred PARSECs (< 400 pc) from the Sun. We collected Gaia DR2 data (G magnitude down to G=19, BP-RP color index, proper motions, and parallaxes) for more than 400 000 stars in a region of 6 degrees on a side, and applied our membership algorithm pyUPMASK. GAIA data for the most probable members was cross-matched with available UBVI data. Finally, we run our ASteCA code to obtain the fundamental cluster parameters.Investigamos la estructura fina del cúmulo abierto NGC 2516. Este es un cúmulo abierto extendido y relativamente joven que subtiende más de dos grados en el cielo, situado a unos pocos cientos de PARSECs (&lt; 400 pc) del Sol. Recopilamos datos de Gaia DR2 (magnitud G hasta G=19, índice de color BP-RP, movimientos propios y paralaje) para más de 400 000 estrellas en una región de 6 grados de lado, y aplicamos nuestro algoritmo de membresía pyUPMASK. Los datos de GAIA para los miembros más probables se correlacionaron con fotometría UBVI. Finalmente, usamos nuestro código ASteCA para obtener los parámetros fundamentales del cúmulo.Asociación Argentina de Astronomía2021info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf122-124http://sedici.unlp.edu.ar/handle/10915/168382enginfo:eu-repo/semantics/altIdentifier/issn/1669-9521info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:36:40Zoai:sedici.unlp.edu.ar:10915/168382Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:36:40.394SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
title Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
spellingShingle Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
Perren, Gabriel Ignacio
Ciencias Astronómicas
galaxies: star clusters: general
open clusters and associations: general
techniques: photometric
methods: statistical
title_short Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
title_full Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
title_fullStr Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
title_full_unstemmed Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
title_sort Fine structure of the main sequence of NGC 2516 scrutinized with Gaia and ASteCA
dc.creator.none.fl_str_mv Perren, Gabriel Ignacio
Giorgi, Edgard Ervar Salvador
Pera, María Sol
Navone, Hugo Daniel
Cruzado, Alicia
Vázquez, Rubén Ángel
author Perren, Gabriel Ignacio
author_facet Perren, Gabriel Ignacio
Giorgi, Edgard Ervar Salvador
Pera, María Sol
Navone, Hugo Daniel
Cruzado, Alicia
Vázquez, Rubén Ángel
author_role author
author2 Giorgi, Edgard Ervar Salvador
Pera, María Sol
Navone, Hugo Daniel
Cruzado, Alicia
Vázquez, Rubén Ángel
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
galaxies: star clusters: general
open clusters and associations: general
techniques: photometric
methods: statistical
topic Ciencias Astronómicas
galaxies: star clusters: general
open clusters and associations: general
techniques: photometric
methods: statistical
dc.description.none.fl_txt_mv The fine structure of the open cluster NGC 2516 is investigated. This is an extended and relatively young open cluster subtending over two degrees in the sky, situated at just a few hundred PARSECs (< 400 pc) from the Sun. We collected Gaia DR2 data (G magnitude down to G=19, BP-RP color index, proper motions, and parallaxes) for more than 400 000 stars in a region of 6 degrees on a side, and applied our membership algorithm pyUPMASK. GAIA data for the most probable members was cross-matched with available UBVI data. Finally, we run our ASteCA code to obtain the fundamental cluster parameters.
Investigamos la estructura fina del cúmulo abierto NGC 2516. Este es un cúmulo abierto extendido y relativamente joven que subtiende más de dos grados en el cielo, situado a unos pocos cientos de PARSECs (&lt; 400 pc) del Sol. Recopilamos datos de Gaia DR2 (magnitud G hasta G=19, índice de color BP-RP, movimientos propios y paralaje) para más de 400 000 estrellas en una región de 6 grados de lado, y aplicamos nuestro algoritmo de membresía pyUPMASK. Los datos de GAIA para los miembros más probables se correlacionaron con fotometría UBVI. Finalmente, usamos nuestro código ASteCA para obtener los parámetros fundamentales del cúmulo.
Asociación Argentina de Astronomía
description The fine structure of the open cluster NGC 2516 is investigated. This is an extended and relatively young open cluster subtending over two degrees in the sky, situated at just a few hundred PARSECs (< 400 pc) from the Sun. We collected Gaia DR2 data (G magnitude down to G=19, BP-RP color index, proper motions, and parallaxes) for more than 400 000 stars in a region of 6 degrees on a side, and applied our membership algorithm pyUPMASK. GAIA data for the most probable members was cross-matched with available UBVI data. Finally, we run our ASteCA code to obtain the fundamental cluster parameters.
publishDate 2021
dc.date.none.fl_str_mv 2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/168382
url http://sedici.unlp.edu.ar/handle/10915/168382
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1669-9521
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
122-124
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.22299

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