FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars

Detalhes bibliográficos
Autor(a) principal: Minniti, Dante
Data de Publicação: 2017
Outros Autores: Palma, Tali, Dékány, István, Hempel, Maren, Rejkuba, Marina, Pullen, Joyce, Alonso Garcia, Javier, Barbá, Rodolfo H., Barbuy, Beatriz, Bica, Eduardo Luiz Damiani, Bonatto, Charles Jose, Borissova, Jura, Catelan, Márcio, Carballo-Bello, Julio A., Chené, André-Nicolas, Claria Olmedo, Juan Jose, Cohen, Roger, Contreras Ramos, Rodrigo, Dias, Bruno Moreira de Souza, Emerson, Jim P., Froebrich, Dirk, Buckner, Anne S. M., Geisler, Doug, Gonzalez, Oscar A., Gran, Felipe, Hajdu, Gergely, Irwin, Michael John, Ivanov, Valentin D., Kurtev, Radostin Georgiev, Lucas, Philip W., Majaess, Daniel J., Mauro, Francesco, Moni Bidin, Christian, Navarrete, Camila, Ramírez Alegría, Sebastián, Saito, Roberto K., Valenti, Elena, Zoccali, Manuela
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/169045
Resumo: We use deep multi-epoch near-IR images of the VISTA Variables in the Vía Láctea (VVV) Survey to search for RR Lyrae stars toward the Southern Galactic plane. Here, we report the discovery of a group of RR Lyrae stars close together in VVV tile d025. Inspection of the VVV images and PSF photometry reveals that most of these stars are likely to belong to a globular cluster that matches the position of the previously known star cluster FSR 1716. The stellar density map of the field yields a >100σ detection for this candidate globular cluster that is centered at equatorial coordinates R.A.J2000 = 16:10:30.0, decl.J2000 = −53:44:56 and galactic coordinates l = 329.77812, b = −1.59227. The color–magnitude diagram of this object reveals a well-populated red giant branch, with a prominent red clump at Ks = 13.35±0.05, and J−Ks = 1.30±0.05. We present the cluster RR Lyrae positions, magnitudes, colors, periods, and amplitudes. The presence of RR Lyrae indicates an old globular cluster, with an age >10 Gyr. We classify this object as an Oosterhoff type I globular cluster, based on the mean period of its RR Lyrae type ab, áPñ = 0.540 days, and argue that this is a relatively metal-poor cluster with [Fe/H] = −1.5±0.4 dex. The mean extinction and reddening for this cluster are AKs = 0.38 0.02 and E( J−Ks) = 0.72±0.02 mag, respectively, as measured from the RR Lyrae colors and the near-IR color– magnitude diagram. We also measure the cluster distance using the RR Lyrae type ab stars. The cluster mean distance modulus is (m−M)0 = 14.38±0.03 mag, implying a distance D = 7.5±0.2 kpc and a Galactocentric distance RG = 4.3 kpc.
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spelling Minniti, DantePalma, TaliDékány, IstvánHempel, MarenRejkuba, MarinaPullen, JoyceAlonso Garcia, JavierBarbá, Rodolfo H.Barbuy, BeatrizBica, Eduardo Luiz DamianiBonatto, Charles JoseBorissova, JuraCatelan, MárcioCarballo-Bello, Julio A.Chené, André-NicolasClaria Olmedo, Juan JoseCohen, RogerContreras Ramos, RodrigoDias, Bruno Moreira de SouzaEmerson, Jim P.Froebrich, DirkBuckner, Anne S. M.Geisler, DougGonzalez, Oscar A.Gran, FelipeHajdu, GergelyIrwin, Michael JohnIvanov, Valentin D.Kurtev, Radostin GeorgievLucas, Philip W.Majaess, Daniel J.Mauro, FrancescoMoni Bidin, ChristianNavarrete, CamilaRamírez Alegría, SebastiánSaito, Roberto K.Valenti, ElenaZoccali, Manuela2017-09-28T02:28:48Z20170004-637Xhttp://hdl.handle.net/10183/169045001026294We use deep multi-epoch near-IR images of the VISTA Variables in the Vía Láctea (VVV) Survey to search for RR Lyrae stars toward the Southern Galactic plane. Here, we report the discovery of a group of RR Lyrae stars close together in VVV tile d025. Inspection of the VVV images and PSF photometry reveals that most of these stars are likely to belong to a globular cluster that matches the position of the previously known star cluster FSR 1716. The stellar density map of the field yields a >100σ detection for this candidate globular cluster that is centered at equatorial coordinates R.A.J2000 = 16:10:30.0, decl.J2000 = −53:44:56 and galactic coordinates l = 329.77812, b = −1.59227. The color–magnitude diagram of this object reveals a well-populated red giant branch, with a prominent red clump at Ks = 13.35±0.05, and J−Ks = 1.30±0.05. We present the cluster RR Lyrae positions, magnitudes, colors, periods, and amplitudes. The presence of RR Lyrae indicates an old globular cluster, with an age >10 Gyr. We classify this object as an Oosterhoff type I globular cluster, based on the mean period of its RR Lyrae type ab, áPñ = 0.540 days, and argue that this is a relatively metal-poor cluster with [Fe/H] = −1.5±0.4 dex. The mean extinction and reddening for this cluster are AKs = 0.38 0.02 and E( J−Ks) = 0.72±0.02 mag, respectively, as measured from the RR Lyrae colors and the near-IR color– magnitude diagram. We also measure the cluster distance using the RR Lyrae type ab stars. The cluster mean distance modulus is (m−M)0 = 14.38±0.03 mag, implying a distance D = 7.5±0.2 kpc and a Galactocentric distance RG = 4.3 kpc.application/pdfengThe astrophysical journal. Bristol. Vol. 838, no. 1 (Mar. 2017), L14, 7 p.Aglomerados globularesFotometria estelarGaláxiasGlobular clusters: generalGalaxies: photometryStars: variables: RR LyraeFSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae starsEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL001026294.pdf001026294.pdfTexto completo (inglês)application/pdf1368727http://www.lume.ufrgs.br/bitstream/10183/169045/1/001026294.pdf521513c9a40c2951c5291143ebffc42aMD51TEXT001026294.pdf.txt001026294.pdf.txtExtracted Texttext/plain34085http://www.lume.ufrgs.br/bitstream/10183/169045/2/001026294.pdf.txt9d61e92317d1166f350b6f4d6b01c450MD52THUMBNAIL001026294.pdf.jpg001026294.pdf.jpgGenerated Thumbnailimage/jpeg2016http://www.lume.ufrgs.br/bitstream/10183/169045/3/001026294.pdf.jpg475ffd8c38637988a85ab7e6e95d4466MD5310183/1690452023-07-15 03:27:58.447176oai:www.lume.ufrgs.br:10183/169045Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-15T06:27:58Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
title FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
spellingShingle FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
Minniti, Dante
Aglomerados globulares
Fotometria estelar
Galáxias
Globular clusters: general
Galaxies: photometry
Stars: variables: RR Lyrae
title_short FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
title_full FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
title_fullStr FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
title_full_unstemmed FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
title_sort FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
author Minniti, Dante
author_facet Minniti, Dante
Palma, Tali
Dékány, István
Hempel, Maren
Rejkuba, Marina
Pullen, Joyce
Alonso Garcia, Javier
Barbá, Rodolfo H.
Barbuy, Beatriz
Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
Borissova, Jura
Catelan, Márcio
Carballo-Bello, Julio A.
Chené, André-Nicolas
Claria Olmedo, Juan Jose
Cohen, Roger
Contreras Ramos, Rodrigo
Dias, Bruno Moreira de Souza
Emerson, Jim P.
Froebrich, Dirk
Buckner, Anne S. M.
Geisler, Doug
Gonzalez, Oscar A.
Gran, Felipe
Hajdu, Gergely
Irwin, Michael John
Ivanov, Valentin D.
Kurtev, Radostin Georgiev
Lucas, Philip W.
Majaess, Daniel J.
Mauro, Francesco
Moni Bidin, Christian
Navarrete, Camila
Ramírez Alegría, Sebastián
Saito, Roberto K.
Valenti, Elena
Zoccali, Manuela
author_role author
author2 Palma, Tali
Dékány, István
Hempel, Maren
Rejkuba, Marina
Pullen, Joyce
Alonso Garcia, Javier
Barbá, Rodolfo H.
Barbuy, Beatriz
Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
Borissova, Jura
Catelan, Márcio
Carballo-Bello, Julio A.
Chené, André-Nicolas
Claria Olmedo, Juan Jose
Cohen, Roger
Contreras Ramos, Rodrigo
Dias, Bruno Moreira de Souza
Emerson, Jim P.
Froebrich, Dirk
Buckner, Anne S. M.
Geisler, Doug
Gonzalez, Oscar A.
Gran, Felipe
Hajdu, Gergely
Irwin, Michael John
Ivanov, Valentin D.
Kurtev, Radostin Georgiev
Lucas, Philip W.
Majaess, Daniel J.
Mauro, Francesco
Moni Bidin, Christian
Navarrete, Camila
Ramírez Alegría, Sebastián
Saito, Roberto K.
Valenti, Elena
Zoccali, Manuela
author2_role author
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author
author
author
author
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author
author
author
author
author
author
author
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dc.contributor.author.fl_str_mv Minniti, Dante
Palma, Tali
Dékány, István
Hempel, Maren
Rejkuba, Marina
Pullen, Joyce
Alonso Garcia, Javier
Barbá, Rodolfo H.
Barbuy, Beatriz
Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
Borissova, Jura
Catelan, Márcio
Carballo-Bello, Julio A.
Chené, André-Nicolas
Claria Olmedo, Juan Jose
Cohen, Roger
Contreras Ramos, Rodrigo
Dias, Bruno Moreira de Souza
Emerson, Jim P.
Froebrich, Dirk
Buckner, Anne S. M.
Geisler, Doug
Gonzalez, Oscar A.
Gran, Felipe
Hajdu, Gergely
Irwin, Michael John
Ivanov, Valentin D.
Kurtev, Radostin Georgiev
Lucas, Philip W.
Majaess, Daniel J.
Mauro, Francesco
Moni Bidin, Christian
Navarrete, Camila
Ramírez Alegría, Sebastián
Saito, Roberto K.
Valenti, Elena
Zoccali, Manuela
dc.subject.por.fl_str_mv Aglomerados globulares
Fotometria estelar
Galáxias
topic Aglomerados globulares
Fotometria estelar
Galáxias
Globular clusters: general
Galaxies: photometry
Stars: variables: RR Lyrae
dc.subject.eng.fl_str_mv Globular clusters: general
Galaxies: photometry
Stars: variables: RR Lyrae
description We use deep multi-epoch near-IR images of the VISTA Variables in the Vía Láctea (VVV) Survey to search for RR Lyrae stars toward the Southern Galactic plane. Here, we report the discovery of a group of RR Lyrae stars close together in VVV tile d025. Inspection of the VVV images and PSF photometry reveals that most of these stars are likely to belong to a globular cluster that matches the position of the previously known star cluster FSR 1716. The stellar density map of the field yields a >100σ detection for this candidate globular cluster that is centered at equatorial coordinates R.A.J2000 = 16:10:30.0, decl.J2000 = −53:44:56 and galactic coordinates l = 329.77812, b = −1.59227. The color–magnitude diagram of this object reveals a well-populated red giant branch, with a prominent red clump at Ks = 13.35±0.05, and J−Ks = 1.30±0.05. We present the cluster RR Lyrae positions, magnitudes, colors, periods, and amplitudes. The presence of RR Lyrae indicates an old globular cluster, with an age >10 Gyr. We classify this object as an Oosterhoff type I globular cluster, based on the mean period of its RR Lyrae type ab, áPñ = 0.540 days, and argue that this is a relatively metal-poor cluster with [Fe/H] = −1.5±0.4 dex. The mean extinction and reddening for this cluster are AKs = 0.38 0.02 and E( J−Ks) = 0.72±0.02 mag, respectively, as measured from the RR Lyrae colors and the near-IR color– magnitude diagram. We also measure the cluster distance using the RR Lyrae type ab stars. The cluster mean distance modulus is (m−M)0 = 14.38±0.03 mag, implying a distance D = 7.5±0.2 kpc and a Galactocentric distance RG = 4.3 kpc.
publishDate 2017
dc.date.accessioned.fl_str_mv 2017-09-28T02:28:48Z
dc.date.issued.fl_str_mv 2017
dc.type.driver.fl_str_mv Estrangeiro
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/169045
dc.identifier.issn.pt_BR.fl_str_mv 0004-637X
dc.identifier.nrb.pt_BR.fl_str_mv 001026294
identifier_str_mv 0004-637X
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url http://hdl.handle.net/10183/169045
dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv The astrophysical journal. Bristol. Vol. 838, no. 1 (Mar. 2017), L14, 7 p.
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eu_rights_str_mv openAccess
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