The high-velocity clouds and the Magellanic Clouds
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 pr...
Guardado en:
| Autor principal: | Olano, Carlos Alberto |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2004
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83503 |
| Aporte de: |
Ejemplares similares
-
Distribution of the high-velocity clouds in the Galactic halo
por: Olano, Carlos Alberto
Publicado: (2008) -
The VISCACHA survey: how star clusters tell the Magellanic Clouds’ history
por: Dias, B., et al.
Publicado: (2022) -
Age-metallicity relation in the Magellanic Clouds clusters
por: Livanou, E., et al.
Publicado: (2013) -
Extended star formation history of the star cluster NGC 2154 in the large magellanic cloud
por: Baume, Gustavo, et al.
Publicado: (2007) -
Five young star clusters in the outer region of the Small Magellanic Cloud
por: Piatti, A.E., et al.