Nuevos estudios espectroscópicos de galaxias IRAS

Observations of four IRAS objects are presented. From their optical spectral characteristics they are classified according to their degree of nuclear activity: two of them as Seyfert 1.9 types and one as an HII region-like galaxy; the remaining one turns out to be a star. Electron temperature and de...

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Autores principales: Agüero, Estela Laura, Suárez Boedo, Fernando E., Paolantonio, Santiago, Calderón, Jesús Humberto
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1994
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/161042
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spelling I19-R120-10915-1610422024-04-30T18:46:20Z http://sedici.unlp.edu.ar/handle/10915/161042 Nuevos estudios espectroscópicos de galaxias IRAS Agüero, Estela Laura Suárez Boedo, Fernando E. Paolantonio, Santiago Calderón, Jesús Humberto 1994 2023-12-04T11:23:08Z es Astronomía Galaxia Observations of four IRAS objects are presented. From their optical spectral characteristics they are classified according to their degree of nuclear activity: two of them as Seyfert 1.9 types and one as an HII region-like galaxy; the remaining one turns out to be a star. Electron temperature and density , and oxygen and nitrogen abundances are given for the HII region-like galaxy. Heliocentric radial velocities are reported too. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
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
Agüero, Estela Laura
Suárez Boedo, Fernando E.
Paolantonio, Santiago
Calderón, Jesús Humberto
Nuevos estudios espectroscópicos de galaxias IRAS
topic_facet Astronomía
Galaxia
description Observations of four IRAS objects are presented. From their optical spectral characteristics they are classified according to their degree of nuclear activity: two of them as Seyfert 1.9 types and one as an HII region-like galaxy; the remaining one turns out to be a star. Electron temperature and density , and oxygen and nitrogen abundances are given for the HII region-like galaxy. Heliocentric radial velocities are reported too.
format Articulo
Comunicacion
author Agüero, Estela Laura
Suárez Boedo, Fernando E.
Paolantonio, Santiago
Calderón, Jesús Humberto
author_facet Agüero, Estela Laura
Suárez Boedo, Fernando E.
Paolantonio, Santiago
Calderón, Jesús Humberto
author_sort Agüero, Estela Laura
title Nuevos estudios espectroscópicos de galaxias IRAS
title_short Nuevos estudios espectroscópicos de galaxias IRAS
title_full Nuevos estudios espectroscópicos de galaxias IRAS
title_fullStr Nuevos estudios espectroscópicos de galaxias IRAS
title_full_unstemmed Nuevos estudios espectroscópicos de galaxias IRAS
title_sort nuevos estudios espectroscópicos de galaxias iras
publishDate 1994
url http://sedici.unlp.edu.ar/handle/10915/161042
work_keys_str_mv AT agueroestelalaura nuevosestudiosespectroscopicosdegalaxiasiras
AT suarezboedofernandoe nuevosestudiosespectroscopicosdegalaxiasiras
AT paolantoniosantiago nuevosestudiosespectroscopicosdegalaxiasiras
AT calderonjesushumberto nuevosestudiosespectroscopicosdegalaxiasiras
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