The high-velocity clouds and the Magellanic Clouds
- Autores
- Olano, Carlos Alberto
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The majority of the high-velocity clouds (HVC) having a common origin linked to the dynamic evolution of the Magellanic Clouds was discussed. It was concluded that the HVC surround the Galaxy, forming a metacloud of ∼300 kpc in size and with a mass of ∼3×109 M⊙. It was found that the HVC were the product of a powerful superwind, which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The effects of the passage of the HVC flow through the Galactic disk produced on the interstellar medium were also analyzed.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Galaxies: interactions
Galaxies: Magellanic Clouds
Galaxy: evolution
Galaxy: halo
Galaxy: structure
ISM: clouds - 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:10915/83503
Ver los metadatos del registro completo
| id |
SEDICI_8725ed6bb226d86b6bf529dd8be94562 |
|---|---|
| oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/83503 |
| network_acronym_str |
SEDICI |
| repository_id_str |
1329 |
| network_name_str |
SEDICI (UNLP) |
| spelling |
The high-velocity clouds and the Magellanic CloudsOlano, Carlos AlbertoCiencias AstronómicasGalaxies: interactionsGalaxies: Magellanic CloudsGalaxy: evolutionGalaxy: haloGalaxy: structureISM: cloudsThe majority of the high-velocity clouds (HVC) having a common origin linked to the dynamic evolution of the Magellanic Clouds was discussed. It was concluded that the HVC surround the Galaxy, forming a metacloud of ∼300 kpc in size and with a mass of ∼3×109 M⊙. It was found that the HVC were the product of a powerful superwind, which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The effects of the passage of the HVC flow through the Galactic disk produced on the interstellar medium were also analyzed.Facultad de Ciencias Astronómicas y Geofísicas2004info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf895-907http://sedici.unlp.edu.ar/handle/10915/83503enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20040177info: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:UNLP2025-10-15T11:07:43Zoai:sedici.unlp.edu.ar:10915/83503Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:07:43.361SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
The high-velocity clouds and the Magellanic Clouds |
| title |
The high-velocity clouds and the Magellanic Clouds |
| spellingShingle |
The high-velocity clouds and the Magellanic Clouds Olano, Carlos Alberto Ciencias Astronómicas Galaxies: interactions Galaxies: Magellanic Clouds Galaxy: evolution Galaxy: halo Galaxy: structure ISM: clouds |
| title_short |
The high-velocity clouds and the Magellanic Clouds |
| title_full |
The high-velocity clouds and the Magellanic Clouds |
| title_fullStr |
The high-velocity clouds and the Magellanic Clouds |
| title_full_unstemmed |
The high-velocity clouds and the Magellanic Clouds |
| title_sort |
The high-velocity clouds and the Magellanic Clouds |
| dc.creator.none.fl_str_mv |
Olano, Carlos Alberto |
| author |
Olano, Carlos Alberto |
| author_facet |
Olano, Carlos Alberto |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: interactions Galaxies: Magellanic Clouds Galaxy: evolution Galaxy: halo Galaxy: structure ISM: clouds |
| topic |
Ciencias Astronómicas Galaxies: interactions Galaxies: Magellanic Clouds Galaxy: evolution Galaxy: halo Galaxy: structure ISM: clouds |
| dc.description.none.fl_txt_mv |
The majority of the high-velocity clouds (HVC) having a common origin linked to the dynamic evolution of the Magellanic Clouds was discussed. It was concluded that the HVC surround the Galaxy, forming a metacloud of ∼300 kpc in size and with a mass of ∼3×109 M⊙. It was found that the HVC were the product of a powerful superwind, which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The effects of the passage of the HVC flow through the Galactic disk produced on the interstellar medium were also analyzed. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
The majority of the high-velocity clouds (HVC) having a common origin linked to the dynamic evolution of the Magellanic Clouds was discussed. It was concluded that the HVC surround the Galaxy, forming a metacloud of ∼300 kpc in size and with a mass of ∼3×109 M⊙. It was found that the HVC were the product of a powerful superwind, which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The effects of the passage of the HVC flow through the Galactic disk produced on the interstellar medium were also analyzed. |
| publishDate |
2004 |
| dc.date.none.fl_str_mv |
2004 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/83503 |
| url |
http://sedici.unlp.edu.ar/handle/10915/83503 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20040177 |
| dc.rights.none.fl_str_mv |
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) |
| eu_rights_str_mv |
openAccess |
| rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
| dc.format.none.fl_str_mv |
application/pdf 895-907 |
| dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
| reponame_str |
SEDICI (UNLP) |
| collection |
SEDICI (UNLP) |
| instname_str |
Universidad Nacional de La Plata |
| instacron_str |
UNLP |
| institution |
UNLP |
| repository.name.fl_str_mv |
SEDICI (UNLP) - Universidad Nacional de La Plata |
| repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
| _version_ |
1846064133479333888 |
| score |
13.22299 |