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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/182035
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T09:35:04Zoai: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:34982025-09-29 09:35:04.761CONICET 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 |
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1844613089059667968 |
score |
13.070432 |