A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae

A study of the available archival IUE images of Beta Lyrae has led the following results: a) for 1250 < λ < 1500 Å, the eclipse depth at the second conjunction is slightly larger than the eclipse depth at primary conjunction; they are equal to 1670 Å; b) the profiles of the resonance lines of...

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Autores principales: Aydin, C., Brandi, Estela, Engin, S., Ferrer, Osvaldo Eduardo, Hack, M., Sahade, Jorge, Solivella, Gladys Rebeca, Yilmaz, N.
Formato: Articulo Comunicacion
Lenguaje:Inglés
Publicado: 1987
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/141446
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id I19-R120-10915-141446
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Galaxia
bet lyr
spellingShingle Astronomía
Galaxia
bet lyr
Aydin, C.
Brandi, Estela
Engin, S.
Ferrer, Osvaldo Eduardo
Hack, M.
Sahade, Jorge
Solivella, Gladys Rebeca
Yilmaz, N.
A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
topic_facet Astronomía
Galaxia
bet lyr
description A study of the available archival IUE images of Beta Lyrae has led the following results: a) for 1250 < λ < 1500 Å, the eclipse depth at the second conjunction is slightly larger than the eclipse depth at primary conjunction; they are equal to 1670 Å; b) the profiles of the resonance lines of Si IV (and the same seems to be true for N V and C IV) can be described as composite, formed by the superposition of a stationary P Cygni profile that suggests a velocity of approach of ∼170 km/s, and a broad, less strong, emission that seems to yield a velocity distribution in antiphase with the velocity curve of the BB II component of the system, suggesting that may be linked with the opaque disk that surrounds the undetected companion; c) the emission lines of the intercombination double of N II at about 2140 Å suggest a velocity of about -130 km/s. The interpretation of the composite profile under b), appears similar to the one suggested by Sahade (1966) to describe Hα and He I 5876 and He I 6678, and by Batten and Sahade (1973) to describe Hα.
format Articulo
Comunicacion
author Aydin, C.
Brandi, Estela
Engin, S.
Ferrer, Osvaldo Eduardo
Hack, M.
Sahade, Jorge
Solivella, Gladys Rebeca
Yilmaz, N.
author_facet Aydin, C.
Brandi, Estela
Engin, S.
Ferrer, Osvaldo Eduardo
Hack, M.
Sahade, Jorge
Solivella, Gladys Rebeca
Yilmaz, N.
author_sort Aydin, C.
title A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
title_short A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
title_full A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
title_fullStr A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
title_full_unstemmed A study of the continuum flux of line structure in the IUE spectrum of Beta Lyrae
title_sort study of the continuum flux of line structure in the iue spectrum of beta lyrae
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/141446
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