Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72)
- Autores
- Piatti, Andres Eduardo; Mestre, Martin Federico; Carballo Bello, Julio A.; Carpintero, Daniel Diego; Navarrete, Camila; Mora, Marcelo D.; Cenzano, Carolina
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the outer regions of the Milky Way globular cluster NGC 6981 based on publicly available BV photometry and new Dark Energy Camera (DECam) observations, both of which reach nearly 4 mag below the cluster main sequence (MS) turnoff. While the BV data sets reveal the present of extra-tidal features around the cluster, the much larger field of view of the DECam observations allowed us to identify some other tidal features, which extend from the cluster toward the opposite direction to the Milky Way center. Such structural features of clusters arise from stellar density maps built using MS stars, following a cleaning of the cluster color-magnitude diagram to remove the contamination of field stars. We also performed N-body simulations in order to help us to understand the spatial distribution of the extra-tidal debris. The outcomes reveal the presence of long trailing and leading tails that are mostly parallel to the direction of the cluster velocity vector. We find that the cluster loses most of its mass by tidal disruption during its perigalactic passages, each of which lasted nearly 20 Myr. Hence, a decrease in the density of escaping stars near the cluster is expected from our N-body simulations, which, in turn, means that stronger extra-tidal features could be found by exploring much larger areas around NGC 6891.
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Fil: Mestre, Martin Federico. 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
Fil: Carballo Bello, Julio A.. Universidad de Tarapacá; Chile
Fil: Carpintero, Daniel Diego. 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
Fil: Navarrete, Camila. Pontificia Universidad Católica de Chile; Chile
Fil: Mora, Marcelo D.. Pontificia Universidad Católica de Chile. Facultad de Física; Chile
Fil: Cenzano, Carolina. Pontificia Universidad Católica de Chile. Facultad de Física; Chile - Materia
-
globular clusters: individual: NGC 6981
techniques: photometric
methods: numerical
Astrophysics of Galaxies - 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:11336/169496
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Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72)Piatti, Andres EduardoMestre, Martin FedericoCarballo Bello, Julio A.Carpintero, Daniel DiegoNavarrete, CamilaMora, Marcelo D.Cenzano, Carolinaglobular clusters: individual: NGC 6981techniques: photometricmethods: numericalAstrophysics of Galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the outer regions of the Milky Way globular cluster NGC 6981 based on publicly available BV photometry and new Dark Energy Camera (DECam) observations, both of which reach nearly 4 mag below the cluster main sequence (MS) turnoff. While the BV data sets reveal the present of extra-tidal features around the cluster, the much larger field of view of the DECam observations allowed us to identify some other tidal features, which extend from the cluster toward the opposite direction to the Milky Way center. Such structural features of clusters arise from stellar density maps built using MS stars, following a cleaning of the cluster color-magnitude diagram to remove the contamination of field stars. We also performed N-body simulations in order to help us to understand the spatial distribution of the extra-tidal debris. The outcomes reveal the presence of long trailing and leading tails that are mostly parallel to the direction of the cluster velocity vector. We find that the cluster loses most of its mass by tidal disruption during its perigalactic passages, each of which lasted nearly 20 Myr. Hence, a decrease in the density of escaping stars near the cluster is expected from our N-body simulations, which, in turn, means that stronger extra-tidal features could be found by exploring much larger areas around NGC 6891.Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaFil: Mestre, Martin Federico. 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; ArgentinaFil: Carballo Bello, Julio A.. Universidad de Tarapacá; ChileFil: Carpintero, Daniel Diego. 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; ArgentinaFil: Navarrete, Camila. Pontificia Universidad Católica de Chile; ChileFil: Mora, Marcelo D.. Pontificia Universidad Católica de Chile. Facultad de Física; ChileFil: Cenzano, Carolina. Pontificia Universidad Católica de Chile. Facultad de Física; ChileEDP Sciences2021-01info: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/11336/169496Piatti, Andres Eduardo; Mestre, Martin Federico; Carballo Bello, Julio A.; Carpintero, Daniel Diego; Navarrete, Camila; et al.; Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72); EDP Sciences; Astronomy and Astrophysics; 646; 1-2021; 176-1840004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202040038info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202040038info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:47:03Zoai:ri.conicet.gov.ar:11336/169496instacron: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 09:47:03.867CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
title |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
spellingShingle |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) Piatti, Andres Eduardo globular clusters: individual: NGC 6981 techniques: photometric methods: numerical Astrophysics of Galaxies |
title_short |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
title_full |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
title_fullStr |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
title_full_unstemmed |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
title_sort |
Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72) |
dc.creator.none.fl_str_mv |
Piatti, Andres Eduardo Mestre, Martin Federico Carballo Bello, Julio A. Carpintero, Daniel Diego Navarrete, Camila Mora, Marcelo D. Cenzano, Carolina |
author |
Piatti, Andres Eduardo |
author_facet |
Piatti, Andres Eduardo Mestre, Martin Federico Carballo Bello, Julio A. Carpintero, Daniel Diego Navarrete, Camila Mora, Marcelo D. Cenzano, Carolina |
author_role |
author |
author2 |
Mestre, Martin Federico Carballo Bello, Julio A. Carpintero, Daniel Diego Navarrete, Camila Mora, Marcelo D. Cenzano, Carolina |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
globular clusters: individual: NGC 6981 techniques: photometric methods: numerical Astrophysics of Galaxies |
topic |
globular clusters: individual: NGC 6981 techniques: photometric methods: numerical Astrophysics of 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 |
We study the outer regions of the Milky Way globular cluster NGC 6981 based on publicly available BV photometry and new Dark Energy Camera (DECam) observations, both of which reach nearly 4 mag below the cluster main sequence (MS) turnoff. While the BV data sets reveal the present of extra-tidal features around the cluster, the much larger field of view of the DECam observations allowed us to identify some other tidal features, which extend from the cluster toward the opposite direction to the Milky Way center. Such structural features of clusters arise from stellar density maps built using MS stars, following a cleaning of the cluster color-magnitude diagram to remove the contamination of field stars. We also performed N-body simulations in order to help us to understand the spatial distribution of the extra-tidal debris. The outcomes reveal the presence of long trailing and leading tails that are mostly parallel to the direction of the cluster velocity vector. We find that the cluster loses most of its mass by tidal disruption during its perigalactic passages, each of which lasted nearly 20 Myr. Hence, a decrease in the density of escaping stars near the cluster is expected from our N-body simulations, which, in turn, means that stronger extra-tidal features could be found by exploring much larger areas around NGC 6891. Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina Fil: Mestre, Martin Federico. 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 Fil: Carballo Bello, Julio A.. Universidad de Tarapacá; Chile Fil: Carpintero, Daniel Diego. 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 Fil: Navarrete, Camila. Pontificia Universidad Católica de Chile; Chile Fil: Mora, Marcelo D.. Pontificia Universidad Católica de Chile. Facultad de Física; Chile Fil: Cenzano, Carolina. Pontificia Universidad Católica de Chile. Facultad de Física; Chile |
description |
We study the outer regions of the Milky Way globular cluster NGC 6981 based on publicly available BV photometry and new Dark Energy Camera (DECam) observations, both of which reach nearly 4 mag below the cluster main sequence (MS) turnoff. While the BV data sets reveal the present of extra-tidal features around the cluster, the much larger field of view of the DECam observations allowed us to identify some other tidal features, which extend from the cluster toward the opposite direction to the Milky Way center. Such structural features of clusters arise from stellar density maps built using MS stars, following a cleaning of the cluster color-magnitude diagram to remove the contamination of field stars. We also performed N-body simulations in order to help us to understand the spatial distribution of the extra-tidal debris. The outcomes reveal the presence of long trailing and leading tails that are mostly parallel to the direction of the cluster velocity vector. We find that the cluster loses most of its mass by tidal disruption during its perigalactic passages, each of which lasted nearly 20 Myr. Hence, a decrease in the density of escaping stars near the cluster is expected from our N-body simulations, which, in turn, means that stronger extra-tidal features could be found by exploring much larger areas around NGC 6891. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-01 |
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/11336/169496 Piatti, Andres Eduardo; Mestre, Martin Federico; Carballo Bello, Julio A.; Carpintero, Daniel Diego; Navarrete, Camila; et al.; Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72); EDP Sciences; Astronomy and Astrophysics; 646; 1-2021; 176-184 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/169496 |
identifier_str_mv |
Piatti, Andres Eduardo; Mestre, Martin Federico; Carballo Bello, Julio A.; Carpintero, Daniel Diego; Navarrete, Camila; et al.; Signatures of tidal disruption in the Milky Way globular cluster NGC 6981 (M72); EDP Sciences; Astronomy and Astrophysics; 646; 1-2021; 176-184 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/url/https://www.aanda.org/10.1051/0004-6361/202040038 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202040038 |
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 |
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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |