Caracteristicas de discos debris en Enanas Blancas

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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: conferenceObject
Lenguaje:Español
Publicado: Asociación Argentina de Astronomıa 2021
Materias:
Enanas blancas
Excesos infrarrojos
Discos de escombros
Distribuciones espectrales de energía
Acceso en línea:http://hdl.handle.net/11086/18980
Aporte de:
Repositorio Digital Universitario (UNC) de Universidad Nacional de Córdoba
id I10-R14111086-18980
record_format dspace
institution Universidad Nacional de Córdoba
institution_str I-10
repository_str R-141
collection Repositorio Digital Universitario (UNC)
language Español
topic Enanas blancas
Excesos infrarrojos
Discos de escombros
Distribuciones espectrales de energía
spellingShingle Enanas blancas
Excesos infrarrojos
Discos de escombros
Distribuciones espectrales de energía
Saker, L
Gómez, Mercedes
Chavero, Carolina Andrea
Caracteristicas de discos debris en Enanas Blancas
topic_facet Enanas blancas
Excesos infrarrojos
Discos de escombros
Distribuciones espectrales de energía
description 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 modeling of the spectral energy distributions (SEDs) of a sample of 29 WDs having IR excesses. This model allows us to derive the mass and the internal and external radii of the dusty disk, for a given chemical composition. The location of this ring is compared with the Habitability Zone (HZ) of each WD in the sample. In addition, the dimensions and masses of these rings are compared with those around main sequence stars, commonly known in the literature as debris disks.
format conferenceObject
author Saker, L
Gómez, Mercedes
Chavero, Carolina Andrea
author_facet Saker, L
Gómez, Mercedes
Chavero, Carolina Andrea
author_sort Saker, L
title Caracteristicas de discos debris en Enanas Blancas
title_short Caracteristicas de discos debris en Enanas Blancas
title_full Caracteristicas de discos debris en Enanas Blancas
title_fullStr Caracteristicas de discos debris en Enanas Blancas
title_full_unstemmed Caracteristicas de discos debris en Enanas Blancas
title_sort caracteristicas de discos debris en enanas blancas
publisher Asociación Argentina de Astronomıa
publishDate 2021
url http://hdl.handle.net/11086/18980
work_keys_str_mv AT sakerl caracteristicasdediscosdebrisenenanasblancas
AT gomezmercedes caracteristicasdediscosdebrisenenanasblancas
AT chaverocarolinaandrea caracteristicasdediscosdebrisenenanasblancas
bdutipo_str Repositorios
_version_ 1764820394738450432

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