Linking the brightest stellar streams with the accretion history of Milky Way like galaxies

Autores
Vera Casanova, Alex; Gómez, Facundo Ariel; Monachesi, Antonela; Gargiulo, Ignacio Daniel; Pallero, Diego; Grand, Robert J. J.; Marinacci, Federico; Pakmor, Rüdiger; Simpson, Christine M.; Frenk, Carlos S.; Morales, Gustavo
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
According to the current galaxy-formation paradigm, mergers and interactions play an important role in shaping present-day galaxies. The remnants of this merger activity can be used to constrain galaxy-formation models. In this work, we use a sample of 30 hydrodynamical simulations of Milky Way mass haloes, from the AURIGA project, to generate surface brightness maps and search for the brightest stream in each halo as a function of varying limiting magnitude. We find that none of the models shows signatures of stellar streams at $mu {r}^{lim} le 25$ mag arcsec-2. The stream detection increases significantly between 28 and 29 mag arcsec-2. Nevertheless, even at 31 mag arcsec-2, 13 per cent of our models show no detectable streams. We study the properties of the brightest streams progenitors (BSPs). We find that BSPs are accreted within a broad range of infall times, from 1.6 to 10 Gyr ago, with only 25 per cent accreted within the last 5 Gyrs; thus, most BSPs correspond to relatively early accretion events. We also find that 37 per cent of the BSPs survive to the present day. The median infall times for surviving and disrupted BSPs are 5.6 and 6.7 Gyr, respectively. We find a clear relation between infall time and infall mass of the BSPs, such that more massive progenitors tend to be accreted at later times. However, we find that the BSPs are not, in most cases, the dominant contributor to the accreted stellar halo of each galaxy.
Fil: Vera Casanova, Alex. Universidad de La Serena; Chile
Fil: Gómez, Facundo Ariel. Universidad de La Serena; Chile
Fil: Monachesi, Antonela. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Gargiulo, Ignacio Daniel. 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: Pallero, Diego. Universidad de La Serena; Chile
Fil: Grand, Robert J. J.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Marinacci, Federico. Universidad de Bologna; Italia
Fil: Pakmor, Rüdiger. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Simpson, Christine M.. University of Chicago; Estados Unidos
Fil: Frenk, Carlos S.. University of Durham; Reino Unido
Fil: Morales, Gustavo. Universidad de La Serena; Chile
Materia
GALAXIES: DWARF
GALAXIES: STRUCTURE
GALAXY: HALO
METHODS: NUMERICAL
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:11336/211736

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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Linking the brightest stellar streams with the accretion history of Milky Way like galaxiesVera Casanova, AlexGómez, Facundo ArielMonachesi, AntonelaGargiulo, Ignacio DanielPallero, DiegoGrand, Robert J. J.Marinacci, FedericoPakmor, RüdigerSimpson, Christine M.Frenk, Carlos S.Morales, GustavoGALAXIES: DWARFGALAXIES: STRUCTUREGALAXY: HALOMETHODS: NUMERICALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1According to the current galaxy-formation paradigm, mergers and interactions play an important role in shaping present-day galaxies. The remnants of this merger activity can be used to constrain galaxy-formation models. In this work, we use a sample of 30 hydrodynamical simulations of Milky Way mass haloes, from the AURIGA project, to generate surface brightness maps and search for the brightest stream in each halo as a function of varying limiting magnitude. We find that none of the models shows signatures of stellar streams at $mu {r}^{lim} le 25$ mag arcsec-2. The stream detection increases significantly between 28 and 29 mag arcsec-2. Nevertheless, even at 31 mag arcsec-2, 13 per cent of our models show no detectable streams. We study the properties of the brightest streams progenitors (BSPs). We find that BSPs are accreted within a broad range of infall times, from 1.6 to 10 Gyr ago, with only 25 per cent accreted within the last 5 Gyrs; thus, most BSPs correspond to relatively early accretion events. We also find that 37 per cent of the BSPs survive to the present day. The median infall times for surviving and disrupted BSPs are 5.6 and 6.7 Gyr, respectively. We find a clear relation between infall time and infall mass of the BSPs, such that more massive progenitors tend to be accreted at later times. However, we find that the BSPs are not, in most cases, the dominant contributor to the accreted stellar halo of each galaxy.Fil: Vera Casanova, Alex. Universidad de La Serena; ChileFil: Gómez, Facundo Ariel. Universidad de La Serena; ChileFil: Monachesi, Antonela. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Gargiulo, Ignacio Daniel. 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: Pallero, Diego. Universidad de La Serena; ChileFil: Grand, Robert J. J.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; AlemaniaFil: Marinacci, Federico. Universidad de Bologna; ItaliaFil: Pakmor, Rüdiger. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; AlemaniaFil: Simpson, Christine M.. University of Chicago; Estados UnidosFil: Frenk, Carlos S.. University of Durham; Reino UnidoFil: Morales, Gustavo. Universidad de La Serena; ChileWiley Blackwell Publishing, Inc2022-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/211736Vera Casanova, Alex; Gómez, Facundo Ariel; Monachesi, Antonela; Gargiulo, Ignacio Daniel; Pallero, Diego; et al.; Linking the brightest stellar streams with the accretion history of Milky Way like galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 4; 8-2022; 4898-49110035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac1636info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:15:03Zoai:ri.conicet.gov.ar:11336/211736instacron: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 10:15:03.429CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
title Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
spellingShingle Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
Vera Casanova, Alex
GALAXIES: DWARF
GALAXIES: STRUCTURE
GALAXY: HALO
METHODS: NUMERICAL
title_short Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
title_full Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
title_fullStr Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
title_full_unstemmed Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
title_sort Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
dc.creator.none.fl_str_mv Vera Casanova, Alex
Gómez, Facundo Ariel
Monachesi, Antonela
Gargiulo, Ignacio Daniel
Pallero, Diego
Grand, Robert J. J.
Marinacci, Federico
Pakmor, Rüdiger
Simpson, Christine M.
Frenk, Carlos S.
Morales, Gustavo
author Vera Casanova, Alex
author_facet Vera Casanova, Alex
Gómez, Facundo Ariel
Monachesi, Antonela
Gargiulo, Ignacio Daniel
Pallero, Diego
Grand, Robert J. J.
Marinacci, Federico
Pakmor, Rüdiger
Simpson, Christine M.
Frenk, Carlos S.
Morales, Gustavo
author_role author
author2 Gómez, Facundo Ariel
Monachesi, Antonela
Gargiulo, Ignacio Daniel
Pallero, Diego
Grand, Robert J. J.
Marinacci, Federico
Pakmor, Rüdiger
Simpson, Christine M.
Frenk, Carlos S.
Morales, Gustavo
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: DWARF
GALAXIES: STRUCTURE
GALAXY: HALO
METHODS: NUMERICAL
topic GALAXIES: DWARF
GALAXIES: STRUCTURE
GALAXY: HALO
METHODS: NUMERICAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv According to the current galaxy-formation paradigm, mergers and interactions play an important role in shaping present-day galaxies. The remnants of this merger activity can be used to constrain galaxy-formation models. In this work, we use a sample of 30 hydrodynamical simulations of Milky Way mass haloes, from the AURIGA project, to generate surface brightness maps and search for the brightest stream in each halo as a function of varying limiting magnitude. We find that none of the models shows signatures of stellar streams at $mu {r}^{lim} le 25$ mag arcsec-2. The stream detection increases significantly between 28 and 29 mag arcsec-2. Nevertheless, even at 31 mag arcsec-2, 13 per cent of our models show no detectable streams. We study the properties of the brightest streams progenitors (BSPs). We find that BSPs are accreted within a broad range of infall times, from 1.6 to 10 Gyr ago, with only 25 per cent accreted within the last 5 Gyrs; thus, most BSPs correspond to relatively early accretion events. We also find that 37 per cent of the BSPs survive to the present day. The median infall times for surviving and disrupted BSPs are 5.6 and 6.7 Gyr, respectively. We find a clear relation between infall time and infall mass of the BSPs, such that more massive progenitors tend to be accreted at later times. However, we find that the BSPs are not, in most cases, the dominant contributor to the accreted stellar halo of each galaxy.
Fil: Vera Casanova, Alex. Universidad de La Serena; Chile
Fil: Gómez, Facundo Ariel. Universidad de La Serena; Chile
Fil: Monachesi, Antonela. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Gargiulo, Ignacio Daniel. 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: Pallero, Diego. Universidad de La Serena; Chile
Fil: Grand, Robert J. J.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Marinacci, Federico. Universidad de Bologna; Italia
Fil: Pakmor, Rüdiger. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Simpson, Christine M.. University of Chicago; Estados Unidos
Fil: Frenk, Carlos S.. University of Durham; Reino Unido
Fil: Morales, Gustavo. Universidad de La Serena; Chile
description According to the current galaxy-formation paradigm, mergers and interactions play an important role in shaping present-day galaxies. The remnants of this merger activity can be used to constrain galaxy-formation models. In this work, we use a sample of 30 hydrodynamical simulations of Milky Way mass haloes, from the AURIGA project, to generate surface brightness maps and search for the brightest stream in each halo as a function of varying limiting magnitude. We find that none of the models shows signatures of stellar streams at $mu {r}^{lim} le 25$ mag arcsec-2. The stream detection increases significantly between 28 and 29 mag arcsec-2. Nevertheless, even at 31 mag arcsec-2, 13 per cent of our models show no detectable streams. We study the properties of the brightest streams progenitors (BSPs). We find that BSPs are accreted within a broad range of infall times, from 1.6 to 10 Gyr ago, with only 25 per cent accreted within the last 5 Gyrs; thus, most BSPs correspond to relatively early accretion events. We also find that 37 per cent of the BSPs survive to the present day. The median infall times for surviving and disrupted BSPs are 5.6 and 6.7 Gyr, respectively. We find a clear relation between infall time and infall mass of the BSPs, such that more massive progenitors tend to be accreted at later times. However, we find that the BSPs are not, in most cases, the dominant contributor to the accreted stellar halo of each galaxy.
publishDate 2022
dc.date.none.fl_str_mv 2022-08
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/11336/211736
Vera Casanova, Alex; Gómez, Facundo Ariel; Monachesi, Antonela; Gargiulo, Ignacio Daniel; Pallero, Diego; et al.; Linking the brightest stellar streams with the accretion history of Milky Way like galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 4; 8-2022; 4898-4911
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/211736
identifier_str_mv Vera Casanova, Alex; Gómez, Facundo Ariel; Monachesi, Antonela; Gargiulo, Ignacio Daniel; Pallero, Diego; et al.; Linking the brightest stellar streams with the accretion history of Milky Way like galaxies; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 4; 8-2022; 4898-4911
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/stac1636
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
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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