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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/168382
Ver los metadatos del registro completo
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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 (< 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:UNLP2025-09-29T11:44:51Zoai: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:13292025-09-29 11:44:52.092SEDICI (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 (< 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 |
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