FSR 1716 : a new Milky Way globular cluster confirmed using VVV RR Lyrae stars
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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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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 author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
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 info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
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 001026294 |
url |
http://hdl.handle.net/10183/169045 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
The astrophysical journal. Bristol. Vol. 838, no. 1 (Mar. 2017), L14, 7 p. |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
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Universidade Federal do Rio Grande do Sul (UFRGS) |
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UFRGS |
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UFRGS |
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Repositório Institucional da UFRGS |
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Repositório Institucional da UFRGS |
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