IRAS Spectra of M-type mira variables

Extinction values for SiC particles obtained in the laboratory by various authors are compared with low-dispersion spectra of M-Mira variables taken by IRAS. The excesses in λ 12 μm and λ 20 μm described by Vardya et al. (1986, Ap.J. Lett. 304, L29), correspond to SiC particle emission of different...

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Detalles Bibliográficos
Autor principal: Minniti, D.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1987
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/137803
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id I19-R120-10915-137803
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Minniti, D.
IRAS Spectra of M-type mira variables
topic_facet Astronomía
Galaxias
description Extinction values for SiC particles obtained in the laboratory by various authors are compared with low-dispersion spectra of M-Mira variables taken by IRAS. The excesses in λ 12 μm and λ 20 μm described by Vardya et al. (1986, Ap.J. Lett. 304, L29), correspond to SiC particle emission of different sizes, which might be related to the shock wave intensities in the atmospheres of these stars.
format Articulo
Comunicacion
author Minniti, D.
author_facet Minniti, D.
author_sort Minniti, D.
title IRAS Spectra of M-type mira variables
title_short IRAS Spectra of M-type mira variables
title_full IRAS Spectra of M-type mira variables
title_fullStr IRAS Spectra of M-type mira variables
title_full_unstemmed IRAS Spectra of M-type mira variables
title_sort iras spectra of m-type mira variables
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/137803
work_keys_str_mv AT minnitid irasspectraofmtypemiravariables
bdutipo_str Repositorios
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