Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars

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Abstract: About 16 % of the main-sequence solar-like stars are surrounded by dusty debris disks (DD). These disks are the detritus of small bodies collisions and their presence is a very strong signpost of planet formation. One of the most interesting characteristics of stars hosting a giant planet...

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Detalles Bibliográficos
Autores principales:	Chavero, Carolina Andrea., Rojas, M., Drake, N. A., Pereira, C. B., Kholtygin, A. F., Cahuasqui, J. A.
Formato:	conferenceObject
Lenguaje:	Inglés
Publicado:	2021
Materias:	Debris disk Chemical abundance Metallicity
Acceso en línea:	http://hdl.handle.net/11086/18938
Aporte de:	Repositorio Digital Universitario (UNC) de Universidad Nacional de Córdoba

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