A search for HI in nine southern galactic clusters
- Autores
- Olano, Carlos Alberto; Pöppel, Wolfgang G. L.; Vota, M. D.
- Año de publicación
- 1980
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The results of a search for H I features in nine galactic clusters are reported. In six of the clusters the earliest spectral types represented are in the range B0–B9. On the whole, twelve H I features (nine maxima and three minima) were detected, of which seven were disregarded as they were not related to any cluster. The conclusion is that at least in six clusters (Cr 121, Cr 140, Cr 132a, b, Ru 3 and Ru 106) no related H I could be detected. For the remainder (NGC 5460, Cr 135 and Cr 394), the evidence was inconclusive. Our results are in agreement with the qualitative conclusion from earlier work that interstellar H I should be expected only in relatively young clusters.
Instituto Argentino de Radioastronomía - Materia
- Astronomía
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/137469
Ver los metadatos del registro completo
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A search for HI in nine southern galactic clustersOlano, Carlos AlbertoPöppel, Wolfgang G. L.Vota, M. D.AstronomíaThe results of a search for H I features in nine galactic clusters are reported. In six of the clusters the earliest spectral types represented are in the range B0–B9. On the whole, twelve H I features (nine maxima and three minima) were detected, of which seven were disregarded as they were not related to any cluster. The conclusion is that at least in six clusters (Cr 121, Cr 140, Cr 132a, b, Ru 3 and Ru 106) no related H I could be detected. For the remainder (NGC 5460, Cr 135 and Cr 394), the evidence was inconclusive. Our results are in agreement with the qualitative conclusion from earlier work that interstellar H I should be expected only in relatively young clusters.Instituto Argentino de Radioastronomía1980info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf247-248http://sedici.unlp.edu.ar/handle/10915/137469enginfo:eu-repo/semantics/altIdentifier/issn/0074-1809info:eu-repo/semantics/altIdentifier/doi/10.1017/s007418090009197xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:23:42Zoai:sedici.unlp.edu.ar:10915/137469Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:23:42.948SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A search for HI in nine southern galactic clusters |
| title |
A search for HI in nine southern galactic clusters |
| spellingShingle |
A search for HI in nine southern galactic clusters Olano, Carlos Alberto Astronomía |
| title_short |
A search for HI in nine southern galactic clusters |
| title_full |
A search for HI in nine southern galactic clusters |
| title_fullStr |
A search for HI in nine southern galactic clusters |
| title_full_unstemmed |
A search for HI in nine southern galactic clusters |
| title_sort |
A search for HI in nine southern galactic clusters |
| dc.creator.none.fl_str_mv |
Olano, Carlos Alberto Pöppel, Wolfgang G. L. Vota, M. D. |
| author |
Olano, Carlos Alberto |
| author_facet |
Olano, Carlos Alberto Pöppel, Wolfgang G. L. Vota, M. D. |
| author_role |
author |
| author2 |
Pöppel, Wolfgang G. L. Vota, M. D. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Astronomía |
| topic |
Astronomía |
| dc.description.none.fl_txt_mv |
The results of a search for H I features in nine galactic clusters are reported. In six of the clusters the earliest spectral types represented are in the range B0–B9. On the whole, twelve H I features (nine maxima and three minima) were detected, of which seven were disregarded as they were not related to any cluster. The conclusion is that at least in six clusters (Cr 121, Cr 140, Cr 132a, b, Ru 3 and Ru 106) no related H I could be detected. For the remainder (NGC 5460, Cr 135 and Cr 394), the evidence was inconclusive. Our results are in agreement with the qualitative conclusion from earlier work that interstellar H I should be expected only in relatively young clusters. Instituto Argentino de Radioastronomía |
| description |
The results of a search for H I features in nine galactic clusters are reported. In six of the clusters the earliest spectral types represented are in the range B0–B9. On the whole, twelve H I features (nine maxima and three minima) were detected, of which seven were disregarded as they were not related to any cluster. The conclusion is that at least in six clusters (Cr 121, Cr 140, Cr 132a, b, Ru 3 and Ru 106) no related H I could be detected. For the remainder (NGC 5460, Cr 135 and Cr 394), the evidence was inconclusive. Our results are in agreement with the qualitative conclusion from earlier work that interstellar H I should be expected only in relatively young clusters. |
| publishDate |
1980 |
| dc.date.none.fl_str_mv |
1980 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/137469 |
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http://sedici.unlp.edu.ar/handle/10915/137469 |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/issn/0074-1809 info:eu-repo/semantics/altIdentifier/doi/10.1017/s007418090009197x |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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