The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)

Autores
Kunder, Andrea; Prudil, Zdenek; Covey, Kevin R.; Hughes, Joanne; Joyce, Meridith; Simion, Iulia T.; Rebekah Kuss; Campos, Carlos; Johnson, Christian I.; Pilachowski, Catherine A.; Larson, Kristen A.; Koch Hansen, Andreas J.; Marchetti, Tommaso; Rich, Michael R.; Butler, Evan; Clarkson, William I.; Rivet, Michael; Devine, Kathryn; Vivas, A. Katherina; Perren, Gabriel Ignacio; Soto, Mario; Silva, Erika
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an indication of the fraction of metal-poor bulge stars that originated from globular clusters can be determined. We observed and analyzed stars in and around BH 261, an understudied globular cluster in the bulge. From seven giants within the tidal radius of the cluster, we measured an average heliocentric radial velocity of 〈RV〉 = −61 ± 2.6 km s−1 with a radial velocity dispersion of 〈σ〉 = 6.1 ± 1.9 km s−1. The large velocity dispersion may have arisen from tidal heating in the cluster´s orbit about the Galactic center, or because BH 261 has a high dynamical mass as well as a high mass-to-light ratio. From spectra of five giants, we measure an average metallicity of 〈[Fe/H]〉 = −1.1 ± 0.2 dex. We also spectroscopically confirm an RR Lyrae star in BH 261, which yields a distance to the cluster of 7.1 ± 0.4 kpc. Stars with 3D velocities and metallicities consistent with BH 261 reaching to ∼05 from the cluster are identified. A handful of these stars are also consistent with the spatial distribution of potential debris from models focusing on the most recent disruption of the cluster.
Fil: Kunder, Andrea. Saint Martinʼs University; Estados Unidos
Fil: Prudil, Zdenek. European Southern Observatory Chile.; Chile
Fil: Covey, Kevin R.. Western Washington University; Estados Unidos
Fil: Hughes, Joanne. Seattle University; Estados Unidos
Fil: Joyce, Meridith. Konkoly Observatory; Hungría
Fil: Simion, Iulia T.. Shanghai Key Lab For Astrophysics; China
Fil: Rebekah Kuss. Oregon State University; Estados Unidos
Fil: Campos, Carlos. Saint Martin's University; Estados Unidos
Fil: Johnson, Christian I.. Space Telescope Science Institute; Estados Unidos
Fil: Pilachowski, Catherine A.. Indiana University; Estados Unidos
Fil: Larson, Kristen A.. Western Washington University.; Estados Unidos
Fil: Koch Hansen, Andreas J.. Astronomisches Rechen-Institut; Alemania
Fil: Marchetti, Tommaso. European Southern Observatory; Alemania
Fil: Rich, Michael R.. University of California at Los Angeles; Estados Unidos
Fil: Butler, Evan. University of Washington; Estados Unidos
Fil: Clarkson, William I.. University of Michigan-Dearborn; Estados Unidos
Fil: Rivet, Michael. Saint Martinʼs University; Estados Unidos
Fil: Devine, Kathryn. The College of Idaho; Estados Unidos
Fil: Vivas, A. Katherina. Cerro Tololo Inter-American Observatory; Chile
Fil: Perren, Gabriel Ignacio. 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: Soto, Mario. Instituto de Astronomía y Ciencias Planetarias; Chile
Fil: Silva, Erika. Western Washington University; Estados Unidos
Materia
STELLAR POPULATIONS
GALACTIC ARCHAEOLOGY
MILKY WAY DYNAMICS
GALACTIC BULGE
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:11336/236734

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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)Kunder, AndreaPrudil, ZdenekCovey, Kevin R.Hughes, JoanneJoyce, MeridithSimion, Iulia T.Rebekah KussCampos, CarlosJohnson, Christian I.Pilachowski, Catherine A.Larson, Kristen A.Koch Hansen, Andreas J.Marchetti, TommasoRich, Michael R.Butler, EvanClarkson, William I.Rivet, MichaelDevine, KathrynVivas, A. KatherinaPerren, Gabriel IgnacioSoto, MarioSilva, ErikaSTELLAR POPULATIONSGALACTIC ARCHAEOLOGYMILKY WAY DYNAMICSGALACTIC BULGEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an indication of the fraction of metal-poor bulge stars that originated from globular clusters can be determined. We observed and analyzed stars in and around BH 261, an understudied globular cluster in the bulge. From seven giants within the tidal radius of the cluster, we measured an average heliocentric radial velocity of 〈RV〉 = −61 ± 2.6 km s−1 with a radial velocity dispersion of 〈σ〉 = 6.1 ± 1.9 km s−1. The large velocity dispersion may have arisen from tidal heating in the cluster´s orbit about the Galactic center, or because BH 261 has a high dynamical mass as well as a high mass-to-light ratio. From spectra of five giants, we measure an average metallicity of 〈[Fe/H]〉 = −1.1 ± 0.2 dex. We also spectroscopically confirm an RR Lyrae star in BH 261, which yields a distance to the cluster of 7.1 ± 0.4 kpc. Stars with 3D velocities and metallicities consistent with BH 261 reaching to ∼05 from the cluster are identified. A handful of these stars are also consistent with the spatial distribution of potential debris from models focusing on the most recent disruption of the cluster.Fil: Kunder, Andrea. Saint Martinʼs University; Estados UnidosFil: Prudil, Zdenek. European Southern Observatory Chile.; ChileFil: Covey, Kevin R.. Western Washington University; Estados UnidosFil: Hughes, Joanne. Seattle University; Estados UnidosFil: Joyce, Meridith. Konkoly Observatory; HungríaFil: Simion, Iulia T.. Shanghai Key Lab For Astrophysics; ChinaFil: Rebekah Kuss. Oregon State University; Estados UnidosFil: Campos, Carlos. Saint Martin's University; Estados UnidosFil: Johnson, Christian I.. Space Telescope Science Institute; Estados UnidosFil: Pilachowski, Catherine A.. Indiana University; Estados UnidosFil: Larson, Kristen A.. Western Washington University.; Estados UnidosFil: Koch Hansen, Andreas J.. Astronomisches Rechen-Institut; AlemaniaFil: Marchetti, Tommaso. European Southern Observatory; AlemaniaFil: Rich, Michael R.. University of California at Los Angeles; Estados UnidosFil: Butler, Evan. University of Washington; Estados UnidosFil: Clarkson, William I.. University of Michigan-Dearborn; Estados UnidosFil: Rivet, Michael. Saint Martinʼs University; Estados UnidosFil: Devine, Kathryn. The College of Idaho; Estados UnidosFil: Vivas, A. Katherina. Cerro Tololo Inter-American Observatory; ChileFil: Perren, Gabriel Ignacio. 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: Soto, Mario. Instituto de Astronomía y Ciencias Planetarias; ChileFil: Silva, Erika. Western Washington University; Estados UnidosIOP Publishing2023-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/236734Kunder, Andrea; Prudil, Zdenek; Covey, Kevin R.; Hughes, Joanne; Joyce, Meridith; et al.; The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3); IOP Publishing; Astronomical Journal; 167; 1; 12-2023; 1-150004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/ad0cfcinfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/ad0cfcinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:47:58Zoai:ri.conicet.gov.ar:11336/236734instacron: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 09:47:59.248CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
title The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
spellingShingle The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
Kunder, Andrea
STELLAR POPULATIONS
GALACTIC ARCHAEOLOGY
MILKY WAY DYNAMICS
GALACTIC BULGE
title_short The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
title_full The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
title_fullStr The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
title_full_unstemmed The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
title_sort The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
dc.creator.none.fl_str_mv Kunder, Andrea
Prudil, Zdenek
Covey, Kevin R.
Hughes, Joanne
Joyce, Meridith
Simion, Iulia T.
Rebekah Kuss
Campos, Carlos
Johnson, Christian I.
Pilachowski, Catherine A.
Larson, Kristen A.
Koch Hansen, Andreas J.
Marchetti, Tommaso
Rich, Michael R.
Butler, Evan
Clarkson, William I.
Rivet, Michael
Devine, Kathryn
Vivas, A. Katherina
Perren, Gabriel Ignacio
Soto, Mario
Silva, Erika
author Kunder, Andrea
author_facet Kunder, Andrea
Prudil, Zdenek
Covey, Kevin R.
Hughes, Joanne
Joyce, Meridith
Simion, Iulia T.
Rebekah Kuss
Campos, Carlos
Johnson, Christian I.
Pilachowski, Catherine A.
Larson, Kristen A.
Koch Hansen, Andreas J.
Marchetti, Tommaso
Rich, Michael R.
Butler, Evan
Clarkson, William I.
Rivet, Michael
Devine, Kathryn
Vivas, A. Katherina
Perren, Gabriel Ignacio
Soto, Mario
Silva, Erika
author_role author
author2 Prudil, Zdenek
Covey, Kevin R.
Hughes, Joanne
Joyce, Meridith
Simion, Iulia T.
Rebekah Kuss
Campos, Carlos
Johnson, Christian I.
Pilachowski, Catherine A.
Larson, Kristen A.
Koch Hansen, Andreas J.
Marchetti, Tommaso
Rich, Michael R.
Butler, Evan
Clarkson, William I.
Rivet, Michael
Devine, Kathryn
Vivas, A. Katherina
Perren, Gabriel Ignacio
Soto, Mario
Silva, Erika
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv STELLAR POPULATIONS
GALACTIC ARCHAEOLOGY
MILKY WAY DYNAMICS
GALACTIC BULGE
topic STELLAR POPULATIONS
GALACTIC ARCHAEOLOGY
MILKY WAY DYNAMICS
GALACTIC BULGE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an indication of the fraction of metal-poor bulge stars that originated from globular clusters can be determined. We observed and analyzed stars in and around BH 261, an understudied globular cluster in the bulge. From seven giants within the tidal radius of the cluster, we measured an average heliocentric radial velocity of 〈RV〉 = −61 ± 2.6 km s−1 with a radial velocity dispersion of 〈σ〉 = 6.1 ± 1.9 km s−1. The large velocity dispersion may have arisen from tidal heating in the cluster´s orbit about the Galactic center, or because BH 261 has a high dynamical mass as well as a high mass-to-light ratio. From spectra of five giants, we measure an average metallicity of 〈[Fe/H]〉 = −1.1 ± 0.2 dex. We also spectroscopically confirm an RR Lyrae star in BH 261, which yields a distance to the cluster of 7.1 ± 0.4 kpc. Stars with 3D velocities and metallicities consistent with BH 261 reaching to ∼05 from the cluster are identified. A handful of these stars are also consistent with the spatial distribution of potential debris from models focusing on the most recent disruption of the cluster.
Fil: Kunder, Andrea. Saint Martinʼs University; Estados Unidos
Fil: Prudil, Zdenek. European Southern Observatory Chile.; Chile
Fil: Covey, Kevin R.. Western Washington University; Estados Unidos
Fil: Hughes, Joanne. Seattle University; Estados Unidos
Fil: Joyce, Meridith. Konkoly Observatory; Hungría
Fil: Simion, Iulia T.. Shanghai Key Lab For Astrophysics; China
Fil: Rebekah Kuss. Oregon State University; Estados Unidos
Fil: Campos, Carlos. Saint Martin's University; Estados Unidos
Fil: Johnson, Christian I.. Space Telescope Science Institute; Estados Unidos
Fil: Pilachowski, Catherine A.. Indiana University; Estados Unidos
Fil: Larson, Kristen A.. Western Washington University.; Estados Unidos
Fil: Koch Hansen, Andreas J.. Astronomisches Rechen-Institut; Alemania
Fil: Marchetti, Tommaso. European Southern Observatory; Alemania
Fil: Rich, Michael R.. University of California at Los Angeles; Estados Unidos
Fil: Butler, Evan. University of Washington; Estados Unidos
Fil: Clarkson, William I.. University of Michigan-Dearborn; Estados Unidos
Fil: Rivet, Michael. Saint Martinʼs University; Estados Unidos
Fil: Devine, Kathryn. The College of Idaho; Estados Unidos
Fil: Vivas, A. Katherina. Cerro Tololo Inter-American Observatory; Chile
Fil: Perren, Gabriel Ignacio. 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: Soto, Mario. Instituto de Astronomía y Ciencias Planetarias; Chile
Fil: Silva, Erika. Western Washington University; Estados Unidos
description The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an indication of the fraction of metal-poor bulge stars that originated from globular clusters can be determined. We observed and analyzed stars in and around BH 261, an understudied globular cluster in the bulge. From seven giants within the tidal radius of the cluster, we measured an average heliocentric radial velocity of 〈RV〉 = −61 ± 2.6 km s−1 with a radial velocity dispersion of 〈σ〉 = 6.1 ± 1.9 km s−1. The large velocity dispersion may have arisen from tidal heating in the cluster´s orbit about the Galactic center, or because BH 261 has a high dynamical mass as well as a high mass-to-light ratio. From spectra of five giants, we measure an average metallicity of 〈[Fe/H]〉 = −1.1 ± 0.2 dex. We also spectroscopically confirm an RR Lyrae star in BH 261, which yields a distance to the cluster of 7.1 ± 0.4 kpc. Stars with 3D velocities and metallicities consistent with BH 261 reaching to ∼05 from the cluster are identified. A handful of these stars are also consistent with the spatial distribution of potential debris from models focusing on the most recent disruption of the cluster.
publishDate 2023
dc.date.none.fl_str_mv 2023-12
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/11336/236734
Kunder, Andrea; Prudil, Zdenek; Covey, Kevin R.; Hughes, Joanne; Joyce, Meridith; et al.; The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3); IOP Publishing; Astronomical Journal; 167; 1; 12-2023; 1-15
0004-6256
CONICET Digital
CONICET
url http://hdl.handle.net/11336/236734
identifier_str_mv Kunder, Andrea; Prudil, Zdenek; Covey, Kevin R.; Hughes, Joanne; Joyce, Meridith; et al.; The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3); IOP Publishing; Astronomical Journal; 167; 1; 12-2023; 1-15
0004-6256
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://iopscience.iop.org/article/10.3847/1538-3881/ad0cfc
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/ad0cfc
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
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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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