A Unique Low-mass-ratio Contact Eclipsing Binary System under the Period Cutoff

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dc.catalogadorkjc
dc.contributor.authorAthanasios Papageorgiou
dc.contributor.authorPanagiota-Eleftheria Christopoulou
dc.contributor.authorEleni Lalounta
dc.contributor.authorC. E. Ferreira Lopes
dc.contributor.authorCatelan , Marcio
dc.contributor.authorAndrew J. Drake
dc.contributor.authorPanayiotis Ηantzios
dc.contributor.authorIoannis Alikakos
dc.date.accessioned2024-03-04T17:01:37Z
dc.date.available2024-03-04T17:01:37Z
dc.date.issued2023
dc.fechaingreso.objetodigital2024-05-16
dc.fuente.origenORCID
dc.identifier.doi10.3847/1538-4357/acdcf3
dc.identifier.urihttps://doi.org/10.3847/1538-4357/acdcf3
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/83642
dc.identifier.wosidWOS:001035376400001
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleA Unique Low-mass-ratio Contact Eclipsing Binary System under the Period Cutoff
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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