Spectral classification of V CrA and Y Mus

Low-dispersion spectra of V CrA and Y Mus are described with some detail. They correspond to hydrogen deficient carbon stars, according to their membership to the R CrB-type variable group. These spectra are classified in the C-system of Keenan and Morgan (1941), following the procedure of Yamashita...

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Detalles Bibliográficos
Autor principal: Minniti, D.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1987
Materias:
Astronomía
Galaxias
v cra
y mus
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/137801
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-137801
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
v cra
y mus
spellingShingle Astronomía
Galaxias
v cra
y mus
Minniti, D.
Spectral classification of V CrA and Y Mus
topic_facet Astronomía
Galaxias
v cra
y mus
description Low-dispersion spectra of V CrA and Y Mus are described with some detail. They correspond to hydrogen deficient carbon stars, according to their membership to the R CrB-type variable group. These spectra are classified in the C-system of Keenan and Morgan (1941), following the procedure of Yamashita(1967). It was found that V CrA and Y Mus are C1,2 and C1,0 respectively. The temperatures derived are in agreement with other determinations.
format Articulo
Comunicacion
author Minniti, D.
author_facet Minniti, D.
author_sort Minniti, D.
title Spectral classification of V CrA and Y Mus
title_short Spectral classification of V CrA and Y Mus
title_full Spectral classification of V CrA and Y Mus
title_fullStr Spectral classification of V CrA and Y Mus
title_full_unstemmed Spectral classification of V CrA and Y Mus
title_sort spectral classification of v cra and y mus
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/137801
work_keys_str_mv AT minnitid spectralclassificationofvcraandymus
bdutipo_str Repositorios
_version_ 1764820457528229889

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