A model for the A2 III3 star with magnetic field: HD 190073

Since the star has a detected magnetic field of about 200 gauss and is observed pole-on, we integrate a velocity law on the basis of theoretical models by Low and Tsinganos. We applied the resulting density distribution to determine the IR free-free radiation (through a model by Lamers and Waters) a...

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Autores principales: Cuttela, Marta, Ringuelet, Adela Emilia
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142559
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id I19-R120-10915-142559
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Cuttela, Marta
Ringuelet, Adela Emilia
A model for the A2 III3 star with magnetic field: HD 190073
topic_facet Astronomía
Galaxia
description Since the star has a detected magnetic field of about 200 gauss and is observed pole-on, we integrate a velocity law on the basis of theoretical models by Low and Tsinganos. We applied the resulting density distribution to determine the IR free-free radiation (through a model by Lamers and Waters) and the continuous absorption. We found that we can explain the IR excess radiation and the discontinuity at λ∼2600.
format Articulo
Comunicacion
author Cuttela, Marta
Ringuelet, Adela Emilia
author_facet Cuttela, Marta
Ringuelet, Adela Emilia
author_sort Cuttela, Marta
title A model for the A2 III3 star with magnetic field: HD 190073
title_short A model for the A2 III3 star with magnetic field: HD 190073
title_full A model for the A2 III3 star with magnetic field: HD 190073
title_fullStr A model for the A2 III3 star with magnetic field: HD 190073
title_full_unstemmed A model for the A2 III3 star with magnetic field: HD 190073
title_sort model for the a2 iii3 star with magnetic field: hd 190073
publishDate 1988
url http://sedici.unlp.edu.ar/handle/10915/142559
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