Some problems associated with large scale galactic structure

The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Galaxy by radio methods. The neutral hydrogen is observed through the 21-cm hyperfine transition line; the continuity of many prominent features indicates that we are seeing the galactic spiral pattern, b...

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Detalles Bibliográficos
Autor principal: Kerr, F.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1969
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/95041
Aporte de:
id I19-R120-10915-95041
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
spellingShingle Astronomía
Galaxias
Kerr, F.
Some problems associated with large scale galactic structure
topic_facet Astronomía
Galaxias
description The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Galaxy by radio methods. The neutral hydrogen is observed through the 21-cm hyperfine transition line; the continuity of many prominent features indicates that we are seeing the galactic spiral pattern, but it is difficult to locate the spiral arms in space because we are restricted to kinematic distance estimates for the hydrogen.
format Articulo
Comunicacion
author Kerr, F.
author_facet Kerr, F.
author_sort Kerr, F.
title Some problems associated with large scale galactic structure
title_short Some problems associated with large scale galactic structure
title_full Some problems associated with large scale galactic structure
title_fullStr Some problems associated with large scale galactic structure
title_full_unstemmed Some problems associated with large scale galactic structure
title_sort some problems associated with large scale galactic structure
publishDate 1969
url http://sedici.unlp.edu.ar/handle/10915/95041
work_keys_str_mv AT kerrf someproblemsassociatedwithlargescalegalacticstructure
bdutipo_str Repositorios
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