A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations

Autores
Oelkers, Ryan J.; Macri, Lucas M.; Marshall, Jennifer L.; DePoy, Darren L.; Colazo, Carlos Roberto; Guzzo, Pablo; Garcia Lambas, Diego Rodolfo; Quiñones, Cecilia; Stringer, Katelyn; Tapia, Luis; Wisdom, Colin
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binary star systems. The vast majority of these systems consist of stars on the main sequence or on the giant branch, leading to a dearth of knowledge of properties at early times (<50 Myr). Only one transiting planet candidate and a dozen eclipsing binaries are known among pre-main sequence objects, yet these are the systems that can provide the best constraints on stellar and planetary formation models. We have recently completed a photometric survey of 3 young (<50 Myr), nearby (D<150 pc) moving groups with a small-aperture instrument, nicknamed ``AggieCam''. We detected 7 candidate Hot Jupiters and over 200 likely pre-main sequence binaries, which are now being followed up photometrically and spectroscopically.
Fil: Oelkers, Ryan J.. Texas A&M University; Estados Unidos
Fil: Macri, Lucas M.. Texas A&M University; Estados Unidos
Fil: Marshall, Jennifer L.. Texas A&M University; Estados Unidos
Fil: DePoy, Darren L.. Texas A&M University; Estados Unidos
Fil: Colazo, Carlos Roberto. 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
Fil: Guzzo, Pablo. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Garcia Lambas, Diego Rodolfo. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. 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
Fil: Quiñones, Cecilia. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Stringer, Katelyn. Texas A&M University; Estados Unidos
Fil: Tapia, Luis. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Wisdom, Colin. Texas A&M University; Estados Unidos
Materia
STARS
SEQUENSE
BINARIES
ECLIPSING
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:11336/182035
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar AssociationsOelkers, Ryan J.Macri, Lucas M.Marshall, Jennifer L.DePoy, Darren L.Colazo, Carlos RobertoGuzzo, PabloGarcia Lambas, Diego RodolfoQuiñones, CeciliaStringer, KatelynTapia, LuisWisdom, ColinSTARSSEQUENSEBINARIESECLIPSINGhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binary star systems. The vast majority of these systems consist of stars on the main sequence or on the giant branch, leading to a dearth of knowledge of properties at early times (<50 Myr). Only one transiting planet candidate and a dozen eclipsing binaries are known among pre-main sequence objects, yet these are the systems that can provide the best constraints on stellar and planetary formation models. We have recently completed a photometric survey of 3 young (<50 Myr), nearby (D<150 pc) moving groups with a small-aperture instrument, nicknamed ``AggieCam''. We detected 7 candidate Hot Jupiters and over 200 likely pre-main sequence binaries, which are now being followed up photometrically and spectroscopically.Fil: Oelkers, Ryan J.. Texas A&M University; Estados UnidosFil: Macri, Lucas M.. Texas A&M University; Estados UnidosFil: Marshall, Jennifer L.. Texas A&M University; Estados UnidosFil: DePoy, Darren L.. Texas A&M University; Estados UnidosFil: Colazo, Carlos Roberto. 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; ArgentinaFil: Guzzo, Pablo. Observatorio Astronomico de la Universidad Nacional de Cordoba; ArgentinaFil: Garcia Lambas, Diego Rodolfo. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. 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; ArgentinaFil: Quiñones, Cecilia. Observatorio Astronomico de la Universidad Nacional de Cordoba; ArgentinaFil: Stringer, Katelyn. Texas A&M University; Estados UnidosFil: Tapia, Luis. Observatorio Astronomico de la Universidad Nacional de Cordoba; ArgentinaFil: Wisdom, Colin. Texas A&M University; Estados UnidosCambridge2016-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/182035Oelkers, Ryan J.; Macri, Lucas M.; Marshall, Jennifer L.; DePoy, Darren L.; Colazo, Carlos Roberto; et al.; A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations; Cambridge; Proceedings of the International Astronomical Union; 10; S314; 1-2016; 73-741743-92131743-9221CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/product/identifier/S1743921315006183/type/journal_articleinfo:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921315006183info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:23:29Zoai:ri.conicet.gov.ar:11336/182035instacron: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:34982025-10-15 14:23:29.4CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
title A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
spellingShingle A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
Oelkers, Ryan J.
STARS
SEQUENSE
BINARIES
ECLIPSING
title_short A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
title_full A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
title_fullStr A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
title_full_unstemmed A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
title_sort A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations
dc.creator.none.fl_str_mv Oelkers, Ryan J.
Macri, Lucas M.
Marshall, Jennifer L.
DePoy, Darren L.
Colazo, Carlos Roberto
Guzzo, Pablo
Garcia Lambas, Diego Rodolfo
Quiñones, Cecilia
Stringer, Katelyn
Tapia, Luis
Wisdom, Colin
author Oelkers, Ryan J.
author_facet Oelkers, Ryan J.
Macri, Lucas M.
Marshall, Jennifer L.
DePoy, Darren L.
Colazo, Carlos Roberto
Guzzo, Pablo
Garcia Lambas, Diego Rodolfo
Quiñones, Cecilia
Stringer, Katelyn
Tapia, Luis
Wisdom, Colin
author_role author
author2 Macri, Lucas M.
Marshall, Jennifer L.
DePoy, Darren L.
Colazo, Carlos Roberto
Guzzo, Pablo
Garcia Lambas, Diego Rodolfo
Quiñones, Cecilia
Stringer, Katelyn
Tapia, Luis
Wisdom, Colin
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv STARS
SEQUENSE
BINARIES
ECLIPSING
topic STARS
SEQUENSE
BINARIES
ECLIPSING
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 past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binary star systems. The vast majority of these systems consist of stars on the main sequence or on the giant branch, leading to a dearth of knowledge of properties at early times (<50 Myr). Only one transiting planet candidate and a dozen eclipsing binaries are known among pre-main sequence objects, yet these are the systems that can provide the best constraints on stellar and planetary formation models. We have recently completed a photometric survey of 3 young (<50 Myr), nearby (D<150 pc) moving groups with a small-aperture instrument, nicknamed ``AggieCam''. We detected 7 candidate Hot Jupiters and over 200 likely pre-main sequence binaries, which are now being followed up photometrically and spectroscopically.
Fil: Oelkers, Ryan J.. Texas A&M University; Estados Unidos
Fil: Macri, Lucas M.. Texas A&M University; Estados Unidos
Fil: Marshall, Jennifer L.. Texas A&M University; Estados Unidos
Fil: DePoy, Darren L.. Texas A&M University; Estados Unidos
Fil: Colazo, Carlos Roberto. 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
Fil: Guzzo, Pablo. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Garcia Lambas, Diego Rodolfo. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. 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
Fil: Quiñones, Cecilia. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Stringer, Katelyn. Texas A&M University; Estados Unidos
Fil: Tapia, Luis. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina
Fil: Wisdom, Colin. Texas A&M University; Estados Unidos
description The past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binary star systems. The vast majority of these systems consist of stars on the main sequence or on the giant branch, leading to a dearth of knowledge of properties at early times (<50 Myr). Only one transiting planet candidate and a dozen eclipsing binaries are known among pre-main sequence objects, yet these are the systems that can provide the best constraints on stellar and planetary formation models. We have recently completed a photometric survey of 3 young (<50 Myr), nearby (D<150 pc) moving groups with a small-aperture instrument, nicknamed ``AggieCam''. We detected 7 candidate Hot Jupiters and over 200 likely pre-main sequence binaries, which are now being followed up photometrically and spectroscopically.
publishDate 2016
dc.date.none.fl_str_mv 2016-01
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/11336/182035
Oelkers, Ryan J.; Macri, Lucas M.; Marshall, Jennifer L.; DePoy, Darren L.; Colazo, Carlos Roberto; et al.; A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations; Cambridge; Proceedings of the International Astronomical Union; 10; S314; 1-2016; 73-74
1743-9213
1743-9221
CONICET Digital
CONICET
url http://hdl.handle.net/11336/182035
identifier_str_mv Oelkers, Ryan J.; Macri, Lucas M.; Marshall, Jennifer L.; DePoy, Darren L.; Colazo, Carlos Roberto; et al.; A wide angle search for hot jupiters and pre-main sequence binaries in Young Stellar Associations; Cambridge; Proceedings of the International Astronomical Union; 10; S314; 1-2016; 73-74
1743-9213
1743-9221
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://www.cambridge.org/core/product/identifier/S1743921315006183/type/journal_article
info:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921315006183
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 Cambridge
publisher.none.fl_str_mv Cambridge
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
_version_ 1846082645676523520
score 13.22299

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