Hα and Hβ Measures as Related to be Star Rotation

Photometric data for the hydrogen lines in 80 southern and 55 northern Be stars give evidence of a constant ratio for the emission in α and β in stars of similar spectral type. In an (α, β) diagram the intersection of this emission-line ratio with the standard relation for non-emission stars gives l...

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Autor principal: Feinstein, Alejandro
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 1975
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/145010
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id I19-R120-10915-145010
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
spellingShingle Astronomía
Feinstein, Alejandro
Hα and Hβ Measures as Related to be Star Rotation
topic_facet Astronomía
description Photometric data for the hydrogen lines in 80 southern and 55 northern Be stars give evidence of a constant ratio for the emission in α and β in stars of similar spectral type. In an (α, β) diagram the intersection of this emission-line ratio with the standard relation for non-emission stars gives lower values than those corresponding to standard stars of the same spectral type. This may be due to rotational effects. A correlation of the variation in the β index with the V magnitude is also given.
format Objeto de conferencia
Objeto de conferencia
author Feinstein, Alejandro
author_facet Feinstein, Alejandro
author_sort Feinstein, Alejandro
title Hα and Hβ Measures as Related to be Star Rotation
title_short Hα and Hβ Measures as Related to be Star Rotation
title_full Hα and Hβ Measures as Related to be Star Rotation
title_fullStr Hα and Hβ Measures as Related to be Star Rotation
title_full_unstemmed Hα and Hβ Measures as Related to be Star Rotation
title_sort hα and hβ measures as related to be star rotation
publishDate 1975
url http://sedici.unlp.edu.ar/handle/10915/145010
work_keys_str_mv AT feinsteinalejandro haandhbmeasuresasrelatedtobestarrotation
bdutipo_str Repositorios
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