The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud

Autores
Ripepi, V.; Marconi, M.; Moretti, M. I.; Clementini, G.; Cioni, M. R. L.; De Grijs, R.; Emerson, J. P.; Groenewegen, M. A. T.; Ivanov, V. D.; Piatti, Andres Eduardo
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The VISTA near-infrared YJK s survey of the Magellanic Clouds System (VMC) is collecting deep K s-band time-series photometry of pulsating variable stars hosted by the two Magellanic Clouds and their connecting Bridge. In this paper, we present Y, J, K s light curves for a sample of 4172 Small Magellanic Cloud (SMC) Classical Cepheids (CCs). These data, complemented with literature V values, allowed us to construct a variety of period-luminosity (PL), period-luminosity-color (PLC), and period-Wesenheit (PW) relationships, which are valid for Fundamental (F), First Overtone (FO), and Second Overtone (SO) pulsators. The relations involving the V, J, K s bands are in agreement with their counterparts in the literature. As for the Y band, to our knowledge, we present the first CC PL, PW, and PLC relations ever derived using this filter. We also present the first near-infrared PL, PW, and PLC relations for SO pulsators to date. We used PW(V, K s) to estimate the relative SMC-LMC distance and, in turn, the absolute distance to the SMC. For the former quantity, we find a value of Δμ = 0.55 -0.04 mag, which is in rather good agreement with other evaluations based on CCs, but significantly larger than the results obtained from older population II distance indicators. This discrepancy might be due to the different geometric distributions of young and old tracers in both Clouds. As for the absolute distance to the SMC, our best estimates are μ SMC = 19.01 -0.05 mag and μ SMC = 19.04 -0.06 mag, based on two distance measurements to the LMC which rely on accurate CC and eclipsing Cepheid binary data, respectively.
Fil: Ripepi, V.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Marconi, M.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Moretti, M. I.. National Observatory of Athens; Grecia. Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing; Grecia
Fil: Clementini, G.. Osservatorio Astronomico di Bologna; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Cioni, M. R. L.. Universitat Potsdam; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. University of Hertfordshire; Reino Unido
Fil: De Grijs, R.. Peking University; China. International Space Science Institute–Beijing; China
Fil: Emerson, J. P.. Queen Mary University of London; Reino Unido
Fil: Groenewegen, M. A. T.. Koninklijke Sterrenwacht van Belgie; Bélgica
Fil: Ivanov, V. D.. European Southern Observatory; Alemania
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Materia
DISTANCE SCALE
MAGELLANIC CLOUDS
STARS: OSCILLATIONS
STARS: VARIABLES: CEPHEIDS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/180447
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The VMC survey. XIX. Classical Cepheids in the Small Magellanic CloudRipepi, V.Marconi, M.Moretti, M. I.Clementini, G.Cioni, M. R. L.De Grijs, R.Emerson, J. P.Groenewegen, M. A. T.Ivanov, V. D.Piatti, Andres EduardoDISTANCE SCALEMAGELLANIC CLOUDSSTARS: OSCILLATIONSSTARS: VARIABLES: CEPHEIDShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1The VISTA near-infrared YJK s survey of the Magellanic Clouds System (VMC) is collecting deep K s-band time-series photometry of pulsating variable stars hosted by the two Magellanic Clouds and their connecting Bridge. In this paper, we present Y, J, K s light curves for a sample of 4172 Small Magellanic Cloud (SMC) Classical Cepheids (CCs). These data, complemented with literature V values, allowed us to construct a variety of period-luminosity (PL), period-luminosity-color (PLC), and period-Wesenheit (PW) relationships, which are valid for Fundamental (F), First Overtone (FO), and Second Overtone (SO) pulsators. The relations involving the V, J, K s bands are in agreement with their counterparts in the literature. As for the Y band, to our knowledge, we present the first CC PL, PW, and PLC relations ever derived using this filter. We also present the first near-infrared PL, PW, and PLC relations for SO pulsators to date. We used PW(V, K s) to estimate the relative SMC-LMC distance and, in turn, the absolute distance to the SMC. For the former quantity, we find a value of Δμ = 0.55 -0.04 mag, which is in rather good agreement with other evaluations based on CCs, but significantly larger than the results obtained from older population II distance indicators. This discrepancy might be due to the different geometric distributions of young and old tracers in both Clouds. As for the absolute distance to the SMC, our best estimates are μ SMC = 19.01 -0.05 mag and μ SMC = 19.04 -0.06 mag, based on two distance measurements to the LMC which rely on accurate CC and eclipsing Cepheid binary data, respectively.Fil: Ripepi, V.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Marconi, M.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Moretti, M. I.. National Observatory of Athens; Grecia. Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing; GreciaFil: Clementini, G.. Osservatorio Astronomico di Bologna; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Cioni, M. R. L.. Universitat Potsdam; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. University of Hertfordshire; Reino UnidoFil: De Grijs, R.. Peking University; China. International Space Science Institute–Beijing; ChinaFil: Emerson, J. P.. Queen Mary University of London; Reino UnidoFil: Groenewegen, M. A. T.. Koninklijke Sterrenwacht van Belgie; BélgicaFil: Ivanov, V. D.. European Southern Observatory; AlemaniaFil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaIOP Publishing2016-07-17info: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/11336/180447Ripepi, V.; Marconi, M.; Moretti, M. I.; Clementini, G.; Cioni, M. R. L.; et al.; The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud; IOP Publishing; Astrophysical Journal Supplement Series; 224; 2; 17-7-2016; 1-240067-00491538-4365CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/0067-0049/224/2/21info:eu-repo/semantics/altIdentifier/doi/10.3847/0067-0049/224/2/21info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1602.09005info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:44:05Zoai:ri.conicet.gov.ar:11336/180447instacron: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 10:44:05.307CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
title The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
spellingShingle The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
Ripepi, V.
DISTANCE SCALE
MAGELLANIC CLOUDS
STARS: OSCILLATIONS
STARS: VARIABLES: CEPHEIDS
title_short The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
title_full The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
title_fullStr The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
title_full_unstemmed The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
title_sort The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud
dc.creator.none.fl_str_mv Ripepi, V.
Marconi, M.
Moretti, M. I.
Clementini, G.
Cioni, M. R. L.
De Grijs, R.
Emerson, J. P.
Groenewegen, M. A. T.
Ivanov, V. D.
Piatti, Andres Eduardo
author Ripepi, V.
author_facet Ripepi, V.
Marconi, M.
Moretti, M. I.
Clementini, G.
Cioni, M. R. L.
De Grijs, R.
Emerson, J. P.
Groenewegen, M. A. T.
Ivanov, V. D.
Piatti, Andres Eduardo
author_role author
author2 Marconi, M.
Moretti, M. I.
Clementini, G.
Cioni, M. R. L.
De Grijs, R.
Emerson, J. P.
Groenewegen, M. A. T.
Ivanov, V. D.
Piatti, Andres Eduardo
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv DISTANCE SCALE
MAGELLANIC CLOUDS
STARS: OSCILLATIONS
STARS: VARIABLES: CEPHEIDS
topic DISTANCE SCALE
MAGELLANIC CLOUDS
STARS: OSCILLATIONS
STARS: VARIABLES: CEPHEIDS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The VISTA near-infrared YJK s survey of the Magellanic Clouds System (VMC) is collecting deep K s-band time-series photometry of pulsating variable stars hosted by the two Magellanic Clouds and their connecting Bridge. In this paper, we present Y, J, K s light curves for a sample of 4172 Small Magellanic Cloud (SMC) Classical Cepheids (CCs). These data, complemented with literature V values, allowed us to construct a variety of period-luminosity (PL), period-luminosity-color (PLC), and period-Wesenheit (PW) relationships, which are valid for Fundamental (F), First Overtone (FO), and Second Overtone (SO) pulsators. The relations involving the V, J, K s bands are in agreement with their counterparts in the literature. As for the Y band, to our knowledge, we present the first CC PL, PW, and PLC relations ever derived using this filter. We also present the first near-infrared PL, PW, and PLC relations for SO pulsators to date. We used PW(V, K s) to estimate the relative SMC-LMC distance and, in turn, the absolute distance to the SMC. For the former quantity, we find a value of Δμ = 0.55 -0.04 mag, which is in rather good agreement with other evaluations based on CCs, but significantly larger than the results obtained from older population II distance indicators. This discrepancy might be due to the different geometric distributions of young and old tracers in both Clouds. As for the absolute distance to the SMC, our best estimates are μ SMC = 19.01 -0.05 mag and μ SMC = 19.04 -0.06 mag, based on two distance measurements to the LMC which rely on accurate CC and eclipsing Cepheid binary data, respectively.
Fil: Ripepi, V.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Marconi, M.. Osservatorio Astronomico di Capodimonte; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Moretti, M. I.. National Observatory of Athens; Grecia. Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing; Grecia
Fil: Clementini, G.. Osservatorio Astronomico di Bologna; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Cioni, M. R. L.. Universitat Potsdam; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. University of Hertfordshire; Reino Unido
Fil: De Grijs, R.. Peking University; China. International Space Science Institute–Beijing; China
Fil: Emerson, J. P.. Queen Mary University of London; Reino Unido
Fil: Groenewegen, M. A. T.. Koninklijke Sterrenwacht van Belgie; Bélgica
Fil: Ivanov, V. D.. European Southern Observatory; Alemania
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
description The VISTA near-infrared YJK s survey of the Magellanic Clouds System (VMC) is collecting deep K s-band time-series photometry of pulsating variable stars hosted by the two Magellanic Clouds and their connecting Bridge. In this paper, we present Y, J, K s light curves for a sample of 4172 Small Magellanic Cloud (SMC) Classical Cepheids (CCs). These data, complemented with literature V values, allowed us to construct a variety of period-luminosity (PL), period-luminosity-color (PLC), and period-Wesenheit (PW) relationships, which are valid for Fundamental (F), First Overtone (FO), and Second Overtone (SO) pulsators. The relations involving the V, J, K s bands are in agreement with their counterparts in the literature. As for the Y band, to our knowledge, we present the first CC PL, PW, and PLC relations ever derived using this filter. We also present the first near-infrared PL, PW, and PLC relations for SO pulsators to date. We used PW(V, K s) to estimate the relative SMC-LMC distance and, in turn, the absolute distance to the SMC. For the former quantity, we find a value of Δμ = 0.55 -0.04 mag, which is in rather good agreement with other evaluations based on CCs, but significantly larger than the results obtained from older population II distance indicators. This discrepancy might be due to the different geometric distributions of young and old tracers in both Clouds. As for the absolute distance to the SMC, our best estimates are μ SMC = 19.01 -0.05 mag and μ SMC = 19.04 -0.06 mag, based on two distance measurements to the LMC which rely on accurate CC and eclipsing Cepheid binary data, respectively.
publishDate 2016
dc.date.none.fl_str_mv 2016-07-17
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/11336/180447
Ripepi, V.; Marconi, M.; Moretti, M. I.; Clementini, G.; Cioni, M. R. L.; et al.; The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud; IOP Publishing; Astrophysical Journal Supplement Series; 224; 2; 17-7-2016; 1-24
0067-0049
1538-4365
CONICET Digital
CONICET
url http://hdl.handle.net/11336/180447
identifier_str_mv Ripepi, V.; Marconi, M.; Moretti, M. I.; Clementini, G.; Cioni, M. R. L.; et al.; The VMC survey. XIX. Classical Cepheids in the Small Magellanic Cloud; IOP Publishing; Astrophysical Journal Supplement Series; 224; 2; 17-7-2016; 1-24
0067-0049
1538-4365
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/10.3847/0067-0049/224/2/21
info:eu-repo/semantics/altIdentifier/doi/10.3847/0067-0049/224/2/21
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1602.09005
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
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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score 13.070432

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