Caracteristicas de discos debris en Enanas Blancas

Abstract: In the late ’80s an infrared excess (IR) around a white dwarf star (WD) was detected, which was attributed to the presence of a dusty circumstellar disk. In recent years, thanks to Spitzer, the number of WDs with excesses has increased significantly. In this contribution we present the mo...

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Detalles Bibliográficos
Autores principales: Saker, L, Gómez, Mercedes, Chavero, Carolina Andrea
Formato: publishedVersion conferenceObject
Lenguaje:Español
Publicado: Asociación Argentina de Astronomıa 2021
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Acceso en línea:http://hdl.handle.net/11086/18980
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